Fix compilation errors and some of the CRITICAL warnings (e9444a97) · Commits · caesar / WP2330 / wiki

docs/source/aspis.rst

+3 −3

Original line number	Diff line number	Diff line
		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.

docs/source/aspis/webapp.rst

+5 −2

Original line number	Diff line number	Diff line
		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

docs/source/caesar.rst

+9 −11

Original line number	Diff line number	Diff line
		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

docs/source/products/data/1A_unitov_mag.rst

+4 −5

Original line number	Diff line number	Diff line
		=========================================
		================================
		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
		-----------------

docs/source/products/data/1B_unitov_vel.rst

+4 −4

Original line number	Diff line number	Diff line
		=========================================
		============================
		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