diff --git a/docs/source/.DS_Store b/docs/source/.DS_Store
deleted file mode 100644
index 5e2895f95244e6493fd593d284d80c029dfe612d..0000000000000000000000000000000000000000
Binary files a/docs/source/.DS_Store and /dev/null differ
diff --git a/docs/source/aspis.rst b/docs/source/aspis.rst
index 510ae99fd348dc039d445bc3418fc2700899d5ce..adf1f2e8a23f155e2578043ce12e0ca2eb433367 100644
--- a/docs/source/aspis.rst
+++ b/docs/source/aspis.rst
@@ -1,6 +1,5 @@
 ASPIS
 =====
-(ASi sPace weather InfraStructure)
 
 The Italian Space Agency has produced a Space Weather (SWE) roadmap **([RD-2])** for a long-term strategy to
 support the future scientific research of SWE, and the development of a related national scientific data centre
@@ -49,9 +48,10 @@ Interactive Archive (MMIA), the SED (Spectral Energy Distribution) Tool and MATI
 .. toctree::
    :caption: ASPIS documentation
 
-   aspis/webapp
-   ASPIS.py library<http://www.example.com/lib/ios/0.1.0/api/>
+   webapp
+   aspis_py
 
 .. autosummary::
    .. toctree:: generated
 
+   ASi sPace weather InfraStructure.
diff --git a/docs/source/aspis/webapp.rst b/docs/source/aspis/webapp.rst
deleted file mode 100644
index 164d48db05115edc2e527f124dbcaa4dd3c95252..0000000000000000000000000000000000000000
--- a/docs/source/aspis/webapp.rst
+++ /dev/null
@@ -1,78 +0,0 @@
-Web Application
----------------
-
-
-Intro
-^^^^^
-
-ASPIS webapp aims to provide an easy, user friendly, access to the data contained in the DATABASE.
-ASPIS webapp will be suited with tools able to easy access and visualize data. Technically, ASPIS
-web-app will access to database using a set of dedicated API (GET) who will act as middleware to the
-Database queries. A key feature will be the function to visualize several data-set in the same page. The
-feature, strongly related to the casual-chain [ref. 1] concept is designed to take into account the standard
-work-flow of the Space Weather community while they are inspecting correlation and liked phenomena
-inside different products. A small and protected amount of server-side and/or client side models should
-be run over visualized data for simple and light computation, notwithstanding the intention of the web-app
-is to facilitate the data exploration and cross-visualization. Users will be encouraged to implement heavy
-computations and advanced data handling using ASPIS.py [ref. 9] libraries.
-
-Functionalities
-^^^^^^^^^^^^^^^
-
-The web-app will be accessible using a common web browser. Basic functionalities are expected to be
-public and will be open to the community:
-
-• Search in the archive based on several keys
-• Time based queries
-• Spatial queries
-• Data visualization
-• Data comparison (Multiple plots)
-• Access to the Causal-chains
-• Causal-chain visualization with multiple plots.
-• Quick citation extraction tools based on visualized data.
-
-Advanced functionalities will be protected and will be accessible only to user identification:
-
-• Save search results
-• Save data visualization settings
-• Run internal, server-side, ASPIS models over an identified data-set
-• (optional) Light computation of model and data comparison
-
-The Access Control List (ACL) will be provided by the ASPIS machines (Fig. 5)
-
-Time-based multi-plot visualization
-...................................
-
-Time is a key link between the most of data-sets provided. So, graphical representation of data shall be
-able to facilitate a time-based comparison between the series visualized by a common timeline. In this
-way, every relationship between time-based plots can be easily found by the user.
-
-Spatial visualization
-.....................
-
-Data-set are generated by instruments spatially referenced by acquisition site (ex. the instrument is
-physically mounted on a Spacecraft or on Earth ), by target position (ex. The instrument target is the
-Sun) and by line of sight (ex. the instrument acquire 20 square deg in a direction of the sky). This info
-can be used to facilitate the user to visualize:
-• Instruments positions in a specified time span
-• Targets positions in a specified time span
-• Targets coverage in instruments line of sights.
-• Visualization of specific phenomena in different reference systems
-
-Event-chain visualization
-.........................
-
-Causal-chains (ref. 1) will get a special section in the webapp. Causal-chains will take advantage from the
-other basic visualization plots and can be associated here as a pre-defined organization of data subsets
-plots. Web-app dedicated section will be able to list and search all causal-chains. Web-app will be able
-to advise the user if, in a nominal visualization plot, the data subset is part of a know causal-chain and
-propose a suitable visualization of such a causal-chain.
-
-Data proximity suggestions
-..........................
-
-User would be prompt by the system in case other data-sets, respect to ones already visualized, will
-have a "proximity" (in terms of observed target, data coherence, data meaning, spatial nearness ) and
-are available in the ASPIS Database system for the observed time-span or in a relevant subsequent time
-(to consider propagation of the phenomena to other instruments).
-
diff --git a/docs/source/caesar.rst b/docs/source/caesar.rst
index 6fc06fa599b4536ae929deb4ec9018b2a3ad4c92..3e17de7964bfac6a3a57ce034ebe26a18348d6b5 100644
--- a/docs/source/caesar.rst
+++ b/docs/source/caesar.rst
@@ -1,29 +1,32 @@
 CAESAR
-======
+=====
 
+.. _intro:
+
+Intro
+-------------
 The Italian Space Agency (ASI) funds the CAESAR_ (Comprehensive spAce wEather Studies for the ASPIS prototype Realization) project.
 The project, officially started on December 21st and lasting 25 months, responds to a call created by the agreement between ASI and the National Institute of Astrophysics (INAF) aimed at carrying out "Study activities for the scientific community of Space Weather for population of the ASPIS scientific data center ".
 
 
-.. _description:
-
-What is CAESAR?
----------------
+.. _description
 
+Description
+----------------
 **CAESAR** (Comprehensive Space Weather Studies for the ASPIS Prototype Realization) is a project supported by the Italian Space Agency and the National Institute of Astrophysics through the ASI-INAF n.2020-35-HH.0 agreement for the development of the ASPIS prototype of scientific data centre for Space Weather. 
 
 .. image:: assets/images/CAESAR_logo_fullsize_color.png
   :height: 220
   :alt: Alternative text
 
-Check out the :doc:`caesar` section for further information, including the details on :ref:`ASPIS` the project.
+Check out the :doc:`CAESAR` section for further information, including the details on :ref:`ASPIS` the project.
 
 To read about the latest news of the project please, visit the website `CAESAR project <https://caesar.iaps.inaf.it>`_
 
-.. _project:
+.. _project
 
 The project
------------
+----------------
 The aim of the project is the creation, within the ASI Space Science Data Center, of a scientific center for the collection, processing and distribution of Space Weather data to the Italian scientific community, called ASPIS_ (ASI Space Weather Infrastructure).
 CAESAR_ will design and build a prototype of ASPIS_ populated with high scientific level data and products.
 
@@ -44,7 +47,6 @@ Prospect...
 
 
 .. _CAESAR: https://caesar.iaps.inaf.it/
-.. _ASPIS: https://www.asi.it
 
 
 
diff --git a/docs/source/index.rst b/docs/source/index.rst
index 2233b2972bd015343d2ec0bec77852330dce23e3..0c576e26b6705e3de38a876731ef62a701ae6216 100644
--- a/docs/source/index.rst
+++ b/docs/source/index.rst
@@ -21,6 +21,8 @@ Contents
    :glob:
 
    aspis
+   webapp
+   aspis_py
    caesar
    products/main
 
@@ -31,12 +33,6 @@ Contents
 
    <hr>
 
-.. toctree::
-   :maxdepth: 4
-   
-   genindex
-   search
-
 
 .. note::
 
diff --git a/docs/source/products/data/.DS_Store b/docs/source/products/data/.DS_Store
deleted file mode 100644
index 5008ddfcf53c02e82d7eee2e57c38e5672ef89f6..0000000000000000000000000000000000000000
Binary files a/docs/source/products/data/.DS_Store and /dev/null differ
diff --git a/docs/source/products/data/1A_unitov_mag.rst b/docs/source/products/data/1A_unitov_mag.rst
deleted file mode 100644
index 697d80494edb3b5de9f9851decaa025135dd67be..0000000000000000000000000000000000000000
--- a/docs/source/products/data/1A_unitov_mag.rst
+++ /dev/null
@@ -1,207 +0,0 @@
-================================
-TSST Full Disk LoS magnetic maps
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-TSST Full Disk LoS magnetic maps
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s.
-
-
-Data Description
-----------------
-
-| **Data type**: image
-
-| **Data formats**: - .fits
-
-
-| **Version**: V1.0
-
-Data Provider
----------------
-
-Data are collected by the following instruments:
-
-- **TSST** - source:
-
-  - MOF
-
-
-
-Data Relationships
-------------------
-
-- type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
-.
-
-Data are ND with - type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
- marked as id: - type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
- - :ref:`- type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
-
-Data Coverage
------------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Photosphere
-
-
-| **Temporal** - time_start: 2022-09-01T15:13:04+02:00
-
-- time_stop: 2023-05-01T15:13:46+02:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-04-29T12:32:27+02:00
-
-| **Last Update**: 2022-04-29T12:32:46+02:00
-
-Data Policy
---------------
-
-This product contains public data. The TSST data are made available freely and without restrictions to all parties and for all purposes exploiting open data policy. As part of the development of collaboration with the broader solar and heliophysics community, however, the TSST team has defined some rules to govern how TSST data should be used. The PI recommends that scientists adhere to the following guidelines: 1) All publications using TSST data should: 1.1) be sent to the PI (luca.giovannelli@roma2.infn.it) after submission to keep record of the relevant publications; 1.2) Acknowledge the sources of data used in all publications, presentations, and reports mentioning the correct DOI of the dataset used in the paper; 1.3) add to the acknowledgments the subsequent text: “The TSST instrument is partially supported by the Italian MIUR-PRIN grant 2017APKP7T on Circumterrestrial Environment: Impact of Sun-Earth Interaction. TSST database is available at: https://helio.roma2.infn.it”;  1.4) where applicable, include the members of the TSST core team (as defined in TSST official website) in the list of authors; 1.5) cite the instrument paper (Giovannelli et al., JSWSC, 2020); 2) In case of any doubt about the instrument, users are encouraged to consult with the PI to discuss the appropriate use of instrument data or derived products..
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file
diff --git a/docs/source/products/data/1B_unitov_vel.rst b/docs/source/products/data/1B_unitov_vel.rst
deleted file mode 100644
index f9cf53931a8be904b1a617136ffc4b99940a47a8..0000000000000000000000000000000000000000
--- a/docs/source/products/data/1B_unitov_vel.rst
+++ /dev/null
@@ -1,208 +0,0 @@
-============================
-TSST Full Disk Velocity Maps
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-TSST Full Disk Velocity Maps
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s.
-
-
-Data Description
-----------------
-
-| **Data type**: image
-
-| **Data formats**: - .fits
-
-
-| **Version**: V1.0
-
-Data Provider
----------------
-
-Data are collected by the following instruments:
-
-- **TSST** - source:
-
-  - MOF
-
-
-
-Data Relationships
-------------------
-
-- type: related-to
-
-- relatedproductid: aspis:///unitov/mag
-
-- relatedproduct: TSST-mag
-
-- description: TSST Full Disk LoS Magnetic Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
-.
-
-Data are ND with - type: related-to
-
-- relatedproductid: aspis:///unitov/mag
-
-- relatedproduct: TSST-mag
-
-- description: TSST Full Disk LoS Magnetic Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
- marked as id: - type: related-to
-
-- relatedproductid: aspis:///unitov/mag
-
-- relatedproduct: TSST-mag
-
-- description: TSST Full Disk LoS Magnetic Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
- - :ref:`- type: related-to
-
-- relatedproductid: aspis:///unitov/mag
-
-- relatedproduct: TSST-mag
-
-- description: TSST Full Disk LoS Magnetic Maps
-
-- type: related-to
-
-- description: TSST H-alpha Full Disk Images
-
-- relatedproduct: TSST-halpha
-
-- relatedproductid: aspis:///unitov/halpha
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
-`
-
-Data Coverage
------------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Photosphere
-
-
-| **Temporal** - time_start: 2022-09-01T15:13:04+02:00
-
-- time_stop: 2023-05-01T15:13:46+02:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-04-29T12:32:27+02:00
-
-| **Last Update**: 2022-04-29T12:32:46+02:00
-
-Data Policy
---------------
-
-This product contains public data. The TSST data are made available freely and without restrictions to all parties and for all purposes exploiting open data policy. As part of the development of collaboration with the broader solar and heliophysics community, however, the TSST team has defined some rules to govern how TSST data should be used. The PI recommends that scientists adhere to the following guidelines: 1) All publications using TSST data should: 1.1) be sent to the PI (luca.giovannelli@roma2.infn.it) after submission to keep record of the relevant publications; 1.2) Acknowledge the sources of data used in all publications, presentations, and reports mentioning the correct DOI of the dataset used in the paper; 1.3) add to the acknowledgments the subsequent text: “The TSST instrument is partially supported by the Italian MIUR-PRIN grant 2017APKP7T on Circumterrestrial Environment: Impact of Sun-Earth Interaction. TSST database is available at: https://helio.roma2.infn.it”;  1.4) where applicable, include the members of the TSST core team (as defined in TSST official website) in the list of authors; 1.5) cite the instrument paper (Giovannelli et al., JSWSC, 2020); 2) In case of any doubt about the instrument, users are encouraged to consult with the PI to discuss the appropriate use of instrument data or derived products..
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file
diff --git a/docs/source/products/data/2_unitov_halpha.rst b/docs/source/products/data/2_unitov_halpha.rst
deleted file mode 100644
index 36863b56da6f4076be710fa459db2f76f7088382..0000000000000000000000000000000000000000
--- a/docs/source/products/data/2_unitov_halpha.rst
+++ /dev/null
@@ -1,208 +0,0 @@
-=============================
-TSST H-alpha Full Disk Images
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-TSST H-alpha Full Disk Images
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-The Hα channel of the TSST is a Daystar SR-127 QT, an achromatic refractor with 127 mm aperture and a focal length of 2667 mm. The telescope features a narrow band filter with a passband of 0.04 nm centered at the Hα line. The filter is a temperature stabilized etalon in collimated configuration, and it is the same filter used in the GONG network for the Hα channel to monitor the chromospheric transients (Giersch, 2013). The Hα channel is equipped with a focal reducer, acting also as a field curvature corrector, to match the Dalsa Pantera 1M60 pixel scale of the MOF channel (2.6 arcsec/pixel). The main goal of this TSST channel is the real time detection of flaring region (Piazzesi et al., 2012; Pötzi et al., 2015, 2018) during the impulsive and flash phases when the intensity reaches its maximum (Benz, 2017). Hα images are extremely important for ground based SWe monitoring (see, e.g. Veronig & Potzi, 2016) and to automatically detect and track structures in the solar chromosphere, as filaments (Bernasconi et al., 2005; Fuller et al., 2005; Bonnin et al., 2013) and prominences (Wang et al., 2010), that can be associated with flare and coronal mass ejections. 
-
-
-Data Description
-----------------
-
-| **Data type**: image
-
-| **Data formats**: - .fits
-
-
-| **Version**: V1.0
-
-Data Provider
--------------
-
-Data are collected by the following instruments:
-
-- **TSST** - source:
-
-  - H-alpha
-
-
-
-Data Relationships
-------------------
-
-- type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST Full Disk LoS magnetic maps
-
-- relatedproduct: TSST-mag
-
-- relatedproductid: aspis:///unitov/mag
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
-.
-
-Data are ND with - type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST Full Disk LoS magnetic maps
-
-- relatedproduct: TSST-mag
-
-- relatedproductid: aspis:///unitov/mag
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
- marked as id: - type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST Full Disk LoS magnetic maps
-
-- relatedproduct: TSST-mag
-
-- relatedproductid: aspis:///unitov/mag
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
- - :ref:`- type: related-to
-
-- relatedproductid: aspis:///unitov/vel
-
-- relatedproduct: TSST-vel
-
-- description: TSST Full Disk Velocity Maps
-
-- type: related-to
-
-- description: TSST Full Disk LoS magnetic maps
-
-- relatedproduct: TSST-mag
-
-- relatedproductid: aspis:///unitov/mag
-
-- type: related-to
-
-- description: TSST Visualization codes
-
-- relatedproduct: TSST-vis-codes
-
-- relatedproductid: aspis:///unitov/vis-codes
-
-- type: related-to
-
-- description: R and D parameters and flare (M- and X-class) probability
-
-- relatedproduct: UNITOV-R-and-D
-
-- relatedproductid: aspis:///unitov/rd
-
-`
-
-Data Coverage
------------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Chromosphere
-
-
-| **Temporal** - time_start: 2022-09-01T15:13:04+02:00
-
-- time_stop: 2023-05-01T15:13:46+02:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-04-29T12:32:27+02:00
-
-| **Last Update**: 2022-04-29T12:32:46+02:00
-
-Data Policy
---------------
-
-This product contains public data. The TSST data are made available freely and without restrictions to all parties and for all purposes exploiting open data policy. As part of the development of collaboration with the broader solar and heliophysics community, however, the TSST team has defined some rules to govern how TSST data should be used. The PI recommends that scientists adhere to the following guidelines: 1) All publications using TSST data should: 1.1) be sent to the PI (luca.giovannelli@roma2.infn.it) after submission to keep record of the relevant publications; 1.2) Acknowledge the sources of data used in all publications, presentations, and reports mentioning the correct DOI of the dataset used in the paper; 1.3) add to the acknowledgments the subsequent text: “The TSST instrument is partially supported by the Italian MIUR-PRIN grant 2017APKP7T on Circumterrestrial Environment: Impact of Sun-Earth Interaction. TSST database is available at: https://helio.roma2.infn.it”;  1.4) where applicable, include the members of the TSST core team (as defined in TSST official website) in the list of authors; 1.5) cite the instrument paper (Giovannelli et al., JSWSC, 2020); 2) In case of any doubt about the instrument, users are encouraged to consult with the PI to discuss the appropriate use of instrument data or derived products..
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file
diff --git a/docs/source/products/data/3_unitov_RandD.rst b/docs/source/products/data/3_unitov_RandD.rst
deleted file mode 100644
index 2f9828d131990fb3967201ad5dd24d1c79e61837..0000000000000000000000000000000000000000
--- a/docs/source/products/data/3_unitov_RandD.rst
+++ /dev/null
@@ -1,80 +0,0 @@
-================================
-R and D Active Region parameters
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-R and D Active Region parameters
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-Parameters for flare-forecasting applications, representing the complexity of a solar active region
-
-
-Data Description
-----------------
-
-| **Data type**: tableset
-
-| **Data formats**: - csv
-
-
-| **Version**: ND
-
-Data Provider
--------------
-
-Data are collected by the following instruments:
-
-- **SDO** - source:
-
-  - HMI
-
-
-
-Data Relationships
-------------------
-
-ND.
-
-Data are ND with ND marked as id: ND - :ref:`ND`
-
-Data Coverage
--------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Photosphere
-
-
-| **Temporal** - time_start: 2012-09-14T03:00:41+02:00
-
-- time_stop: 2016-04-13T12:01:00+02:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-05-11T10:59:38+02:00
-
-| **Last Update**: 2022-05-11T10:59:42+02:00
-
-Data Policy
---------------
-
-This product contains public data. Other.
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file
diff --git a/docs/source/products/data/48D_ingv_LMPalert.rst b/docs/source/products/data/48D_ingv_LMPalert.rst
deleted file mode 100644
index d98520a633cc396ff280fba4af300bbad4a21191..0000000000000000000000000000000000000000
--- a/docs/source/products/data/48D_ingv_LMPalert.rst
+++ /dev/null
@@ -1,113 +0,0 @@
-=========================
-Lampedusa GIC level alert
-~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-Lampedusa GIC level alert
-~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-From both components of GIC index for Lampedusa observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data)
-
-
-Data Description
-----------------
-
-| **Data type**: timeseries
-
-| **Data formats**: - json
-- txt
-
-
-| **Version**: ND
-
-Data Provider
--------------
-
-Data are collected by the following instruments:
-
-- **INGV** - source:
-
-  - Algorithm
-
-
-
-Data Relationships
-------------------
-
-- type: related-to
-
-- description: input data needed to calculate GIC level alert
-
-- relatedproduct: Lampedusa GIC index
-
-- relatedproductid: LMPGIC
-
-.
-
-Data are ND with - type: related-to
-
-- description: input data needed to calculate GIC level alert
-
-- relatedproduct: Lampedusa GIC index
-
-- relatedproductid: LMPGIC
-
- marked as id: - type: related-to
-
-- description: input data needed to calculate GIC level alert
-
-- relatedproduct: Lampedusa GIC index
-
-- relatedproductid: LMPGIC
-
- - :ref:`- type: related-to
-
-- description: input data needed to calculate GIC level alert
-
-- relatedproduct: Lampedusa GIC index
-
-- relatedproductid: LMPGIC
-
-`
-
-Data Coverage
------------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Earth's Ground
-
-
-| **Temporal** - time_start: 2017-04-04T00:00:00+01:00
-
-- time_stop: 2022-04-21T00:00:00+02:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-04-30T18:00:00+02:00
-
-| **Last Update**: 2022-04-30T18:00:00+02:00
-
-Data Policy
---------------
-
-This product contains public data. Not defined.
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file
diff --git a/docs/source/products/data/49A_ingv_Swarm_LoL_maps.rst b/docs/source/products/data/49A_ingv_Swarm_LoL_maps.rst
deleted file mode 100644
index f9e8c2ce282dc0b740c8cb600cdc92841968e0b9..0000000000000000000000000000000000000000
--- a/docs/source/products/data/49A_ingv_Swarm_LoL_maps.rst
+++ /dev/null
@@ -1,118 +0,0 @@
-===================================================================
-GPS Loss of Lock (LoL) events global maps from ESA Swarm satellites
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-GPS Loss of Lock (LoL) events global maps from ESA Swarm satellites
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-Global maps of GPS LoL (Loss of Lock) events, as derived by total electron content observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020.
-
-
-Data Description
-----------------
-
-| **Data type**: image
-
-| **Data formats**: - text files
-
-
-| **Version**: ND
-
-Data Provider
--------------
-
-Data are collected by the following instruments:
-
-- **Swarm A satellite** - source:
-
-  - ESA Swarm A Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/
-- **Swarm B satellite** - source:
-
-  - ESA Swarm B Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/
-- **Swarm C satellite** - source:
-
-  - ESA Swarm C Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/
-
-
-
-Data Relationships
-------------------
-
-- type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproduct: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
-.
-
-Data are ND with - type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproduct: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
- marked as id: - type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproduct: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
- - :ref:`- type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproduct: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
-`
-
-Data Coverage
------------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Earth's Ionosphere
-
-
-| **Temporal** - time_start: 2014-01-01T00:00:50+01:00
-
-- time_stop: 2020-12-31T23:59:07+01:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-04-26T16:16:20+02:00
-
-| **Last Update**: 2022-04-26T17:05:28+02:00
-
-Data Policy
---------------
-
-This product contains public data. Images available upon request or database query.
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file
diff --git a/docs/source/products/data/49B_ingv_Swarm_LoL_ts.rst b/docs/source/products/data/49B_ingv_Swarm_LoL_ts.rst
deleted file mode 100644
index a869cfcda314796da65b79f86df7bbf8c1608fef..0000000000000000000000000000000000000000
--- a/docs/source/products/data/49B_ingv_Swarm_LoL_ts.rst
+++ /dev/null
@@ -1,118 +0,0 @@
-===================================================================
-GPS Loss of Lock (LoL) events time series from ESA Swarm satellites
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-=========================================
-
-.. sectnum::
-
-.. contents:: The tiny table of contents
-
-GPS Loss of Lock (LoL) events time series from ESA Swarm satellites
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-
-GPS LoL (Loss of Lock) events, as derived by total electron content observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020.
-
-
-Data Description
-----------------
-
-| **Data type**: tableset
-
-| **Data formats**: - text files
-
-
-| **Version**: ND
-
-Data Provider
--------------
-
-Data are collected by the following instruments:
-
-- **Swarm A satellite** - source:
-
-  - ESA Swarm A Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/
-- **Swarm B satellite** - source:
-
-  - ESA Swarm B Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/
-- **Swarm C satellite** - source:
-
-  - ESA Swarm C Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/
-
-
-
-Data Relationships
-------------------
-
-- type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
-- relatedproduct: Global maps of ionospheric indices
-
-.
-
-Data are ND with - type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
-- relatedproduct: Global maps of ionospheric indices
-
- marked as id: - type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
-- relatedproduct: Global maps of ionospheric indices
-
- - :ref:`- type: related-to
-
-- description: Global maps of ionospheric indices
-
-- relatedproductid: 32
-
-- relatedproduct: Global maps of ionospheric indices
-
-`
-
-Data Coverage
--------------
-The product cover measurements for the ND messangers.
-
-Data coverage is listed below:
-
-| **Spatial** - Earth's Ionosphere
-
-
-| **Temporal** - time_start: 2014-01-01T00:00:50+01:00
-
-- time_stop: 2020-12-31T23:59:07+01:00
-
-
-
-| **Spectral** range: ND ND -  ND ND 
-
-Product Status
----------------
-
-| **Status**: Active
-
-| **Creation date**: 2022-04-26T16:16:20+02:00
-
-| **Last Update**: 2022-04-26T17:05:28+02:00
-
-Data Policy
---------------
-
-This product contains public data. Time series in .txt format available upon request or database query.
-
-Example
-------------
-
-Example is not yet provided .
\ No newline at end of file