Fix compilation errors and some of the CRITICAL warnings

e9444a97 · Valerio Formato · 77a8fba8 · e9444a97 · e9444a97 · e9444a97
Commit e9444a97 authored Oct 30, 2023 by Valerio Formato
--- a/docs/source/aspis.rst
+++ b/docs/source/aspis.rst
 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
@@ -28,7 +29,7 @@ discover, understand, and model the connection between solar phenomena, interpla
 their impacts on the planets (especially the Earth).
 ASI-SSDC context
------------
+----------------
 The Space Science Data Center of the Italian Space Agency has its roots in the early ’90s with the Data Center of
 the BeppoSax X-ray astronomy satellite, then evolved into the ASI Science Data Center (ASDC), established in
@@ -54,4 +55,3 @@ Interactive Archive (MMIA), the SED (Spectral Energy Distribution) Tool and MATI
 .. autosummary::
   .. toctree:: generated
-   ASi sPace weather InfraStructure.
--- a/docs/source/aspis/webapp.rst
+++ b/docs/source/aspis/webapp.rst
 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
@@ -30,11 +30,14 @@ public and will be open to the community:
 • 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

--- a/docs/source/caesar.rst
+++ b/docs/source/caesar.rst
 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
+.. _description:
+What is CAESAR?
+---------------
-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.
@@ -47,6 +44,7 @@ Prospect...
 .. _CAESAR: https://caesar.iaps.inaf.it/
+.. _ASPIS: https://www.asi.it

--- a/docs/source/products/data/1A_unitov_mag.rst
+++ b/docs/source/products/data/1A_unitov_mag.rst
-=========================================
+================================
 TSST Full Disk LoS magnetic maps
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ TSST Full Disk LoS magnetic maps
 .. 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.
@@ -37,7 +37,7 @@ Data are collected by the following instruments:
 Data Relationships
-----------------
+------------------
 - type: related-to
@@ -169,7 +169,6 @@ Data are ND with - type: related-to
 - relatedproductid: aspis:///unitov/rd
-`
 Data Coverage
 -----------------

--- a/docs/source/products/data/1B_unitov_vel.rst
+++ b/docs/source/products/data/1B_unitov_vel.rst
-=========================================
+============================
 TSST Full Disk Velocity Maps
-~~~~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ TSST Full Disk Velocity Maps
 .. 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.
@@ -37,7 +37,7 @@ Data are collected by the following instruments:
 Data Relationships
-----------------
+------------------
 - type: related-to

--- a/docs/source/products/data/2_unitov_halpha.rst
+++ b/docs/source/products/data/2_unitov_halpha.rst
-=========================================
+=============================
 TSST H-alpha Full Disk Images
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ TSST H-alpha Full Disk Images
 .. 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. 
@@ -26,7 +26,7 @@ Data Description
 | **Version**: V1.0
 Data Provider
---------------
+-------------
 Data are collected by the following instruments:
@@ -37,7 +37,7 @@ Data are collected by the following instruments:
 Data Relationships
-----------------
+------------------
 - type: related-to

--- a/docs/source/products/data/3_unitov_RandD.rst
+++ b/docs/source/products/data/3_unitov_RandD.rst
-=========================================
+================================
 R and D Active Region parameters
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ R and D Active Region parameters
 .. 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
@@ -26,7 +26,7 @@ Data Description
 | **Version**: ND
 Data Provider
---------------
+-------------
 Data are collected by the following instruments:
@@ -37,14 +37,14 @@ Data are collected by the following instruments:
 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:

--- a/docs/source/products/data/48D_ingv_LMPalert.rst
+++ b/docs/source/products/data/48D_ingv_LMPalert.rst
-=========================================
+=========================
 Lampedusa GIC level alert
-~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ Lampedusa GIC level alert
 .. 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)
@@ -27,7 +27,7 @@ Data Description
 | **Version**: ND
 Data Provider
---------------
+-------------
 Data are collected by the following instruments:
@@ -38,7 +38,7 @@ Data are collected by the following instruments:
 Data Relationships
-----------------
+------------------
 - type: related-to

--- a/docs/source/products/data/49A_ingv_Swarm_LoL_maps.rst
+++ b/docs/source/products/data/49A_ingv_Swarm_LoL_maps.rst
-=========================================
+===================================================================
 GPS Loss of Lock (LoL) events global maps from ESA Swarm satellites
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ GPS Loss of Lock (LoL) events global maps from ESA Swarm satellites
 .. 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.
@@ -26,7 +26,7 @@ Data Description
 | **Version**: ND
 Data Provider
---------------
+-------------
 Data are collected by the following instruments:
@@ -43,7 +43,7 @@ Data are collected by the following instruments:
 Data Relationships
-----------------
+------------------
 - type: related-to

--- a/docs/source/products/data/49B_ingv_Swarm_LoL_ts.rst
+++ b/docs/source/products/data/49B_ingv_Swarm_LoL_ts.rst
-=========================================
+===================================================================
 GPS Loss of Lock (LoL) events time series from ESA Swarm satellites
-~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
 =========================================
@@ -9,7 +9,7 @@ GPS Loss of Lock (LoL) events time series from ESA Swarm satellites
 .. 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.
@@ -26,7 +26,7 @@ Data Description
 | **Version**: ND
 Data Provider
---------------
+-------------
 Data are collected by the following instruments:
@@ -43,7 +43,7 @@ Data are collected by the following instruments:
 Data Relationships
-----------------
+------------------
 - type: related-to
@@ -82,7 +82,7 @@ Data are ND with - type: related-to
 `
 Data Coverage
-----------------
+-------------
 The product cover measurements for the ND messangers.
 Data coverage is listed below: