Publisher: IDOC - STScI NAVO Directory Search Results

ID:: ivo://idoc/__system__/adql/query
Title:: ADQL Query
Short Name:: gavoadql
Date:: 12 Mar 2021 16:02:22
Publisher:: IDOC
Description:: An endpoint for submitting ADQL queries to the data center and retrieving the result in various forms.

ID:: ivo://idoc/medoc/eit_syn/q/epn_core
Title:: EUV-SYN
Short Name:: eit_syn.epn_core
Date:: 16 Nov 2023 13:44:59
Publisher:: IDOC
Description:: *** EUV-SYN *** Synchronous synoptic maps of the corona in the extreme-UV (EUV), built from series of SoHO/EIT observations, in each of the 4 wavelength bands of the instrument. Synchronous synoptic maps are maps of the EUV radiance in different wavelength bands on the full solar sphere, in heliographic (Carrington) longitude and latitude, where data are taken as close as possible to a reference time. They capture the state of the corona at any given reference time by including data taken as close as possible to this time. EUV-SYN is available as part of the generic MEDOC interface which is currently located at https://idoc-medoc.ias.u-psud.fr/. These interfaces are based on the CNES SiTools2 framework. EUV-SYN is also available from IDL and Python scripts, using a specialization of the generic SiTools2 IDL and Python clients developed by MEDOC.

ID:: ivo://idoc.ginco
Title:: GINCO: Galaxy, INterstellar matter and Cosmology
Short Name:: GINCO
Date:: 16 May 2019 14:25:55
Publisher:: IDOC
Description:: GINCO is a center for expertise for several space, balloon and ground mission. It has an important role in data processing, distribution and interpretation, for several astronomy missions at long wavelength. In this matter, GINCO : develops and maintains high level analysis pipelines develops and maintains data archives & access develops, maintains and distribute high level software for data analysis offers scientific expertise for mission using long wavelength detectors plays an important role in education and outreach to the general public

ID:: ivo://idoc/tap
Title:: IDOC: Integrated Data and Operating Center TAP service
Short Name:: IDOC TAP
Date:: 16 Nov 2023 16:51:52
Publisher:: IDOC
Description:: The IDOC: Integrated Data and Operating Center's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: epn_core from the eit_syn schema, epn_core from the gaia_dem schema, epn_core from the omega_cubes schema, epn_core from the omega_maps schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.

ID:: ivo://idoc
Title:: Integrated Data and Operation Center
Short Name:: IDOC
Date:: 08 Mar 2021 11:57:05
Publisher:: IDOC
Description:: IDOC (Integrated Data and Operation Center) is located and operated at IAS, Orsay, France under contract with CNRS, CNES, and Univ. Paris-Sud.IDOC takes part in all the operational phases of space missions.\ These thematic data centers span a large area in solar physics with MEDOC, in planetary science with PSUP, in exo planetolgy with D2S and in astronomy with GINCO.\ IDOC belongs to the Paris Sud Observatory (OSU).

ID:: ivo://idoc/medoc/gaia_dem/q/epn_core
Title:: SDO GAIA-DEM
Short Name:: gaia_dem.epn_cor
Date:: 30 Nov 2023 19:23:40
Publisher:: IDOC
Description:: <b>GAIA-DEM</b><br/> GAIA-DEM is a database of Differential Emission Measure (DEM) maps. The DEM is a measure of the thermal structure of the coronal plasma, representing the quantity of light emitting plasma along the line of sight, at different temperatures. In GAIA-DEM, the DEM is modelled by a specific function of temperature, namely a Gaussian of the logarithm of electron temperature. GAIA-DEM maps are then maps of the DEM maximum temperature, of the DEM integral (total Emission Measure), and DEM width (in temperature). These maps are obtained by inversion from the SDO/AIA EUV images in 6 coronal channels (9.4, 13.1, 17.1, 19.3, 21.1, and 33.5 nm). In addition, maps of the χ² for the inversion are provided.<br/> GAIA-DEM is available from a specific interface at <a href="http://medoc-dem.ias.u-psud.fr/">http://medoc-dem.ias.u-psud.fr</a>, as well as part of the generic MEDOC interface which is currently located at <a href="https://idoc-medoc.ias.u-psud.fr/">https://idoc-medoc.ias.u-psud.fr</a>. These interfaces are based on the CNES SiTools2 framework. GAIA-DEM is also available from IDL and Python scripts, using a specialization of the generic SiTools2 IDL and Python clients developed by MEDOC.

ID:: ivo://idoc/q/epn_core
Title:: SDO GAIA-DEM
Date:: 08 Dec 2021 14:22:45
Publisher:: IDOC
Description:: *** GAIA-DEM *** GAIA-DEM is a database of Differential Emission Measure (DEM) maps. The DEM is a measure of the thermal structure of the coronal plasma, representing the quantity of light emitting plasma along the line of sight, at different temperatures. In GAIA-DEM, the DEM is modelled by a specific function of temperature, namely a Gaussian of the logarithm of electron temperature. GAIA-DEM maps are then maps of the DEM maximum temperature, of the DEM integral (total Emission Measure), and DEM width (in temperature). These maps are obtained by inversion from the SDO/AIA EUV images in 6 coronal channels (9.4, 13.1, 17.1, 19.3, 21.1, and 33.5nm). In addition, maps of the ÏÂ² for the inversion are provided. GAIA-DEM is available from a specific interface at http://medoc-dem.ias.u-psud.fr/, as well as part of the generic MEDOC interface which is currently located at http://idocmedoc- test.ias.u-psud.fr/. These interfaces are based on the CNES SiTools2 framework. GAIA-DEM is also available from IDL and Python scripts, using a specialization of the generic SiTools2 IDL and Python clients developed by MEDOC.

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