diff --git a/docs/source/aspis_py.rst b/docs/source/aspis_py.rst
index eeee9178c0ffc3df78469c27aad3413a8b541f9b..ad37817f0152b962b785b158632d271c0c5108ab 100644
--- a/docs/source/aspis_py.rst
+++ b/docs/source/aspis_py.rst
@@ -1,14 +1,14 @@
-ASPIS.py library
+ASPIS.py package
 ----------------
 
 Intro
 ^^^^^
 
-ASPIS.py is a library of code that allows access to the data contained in ASPIS database and other
+ASPIS.py is a package of code that allows access to the data contained in ASPIS database and other
 various community databases, to perform client-side specific analyses of this data and to
 visualize it. The data available are of two types: data in the internal database produced by the CAESAR
 community and information on external data in other databases. Along with access to the data, the
-ASPIS.py library contains code packages that can be imported as library objects, with which to perform
+ASPIS.py package contains code packages that can be imported as package objects, with which to perform
 analysis and/or visualization of the data.
 
 The criterion of ASPIS.py is to act as a collector for the data and analysis software of the Space Weather (SWx) Italian
@@ -25,7 +25,7 @@ standardization, making it easier for researchers to work with and build upon ea
 field of SWX and astrophysics in general.
 
 Functions
-^^^^^^^^^^^^^^^^^^
+^^^^^^^^^
 
 The functions of the ASPIS.py module are conceived to implement the following key components of the
 ASPIS service:
@@ -94,7 +94,7 @@ the provided Wheel file. Note that version number may have changed.
 Use case example
 ^^^^^^^^^^^^^^^^
 
-Here we show an example of the way a user can use a specific product of the ASPIS.py library.
+Here we show an example of the way a user can use a specific product of the ASPIS.py package.
 from aspis import products as aps
 from datetime import datetime
 
@@ -128,7 +128,7 @@ plot:
 
 This example code performs the following steps:
 
-#.  Import necessary modules and classes from the "aspis" library.
+#.  Import necessary modules and classes from the "aspis" package.
 #.  Define input parameters, namely the initial velocity (V0), its uncertainty (sigma_V0), and a times-tamp (Time_UTC).
 #.  Create an instance of the "pdbm" class from the "aspis.products" module.
 #.  Use this instance to compute the CME (Coronal Mass Ejection) model parameters based on the provided input.