Content Level: General / Validation Level: 2 - STScI NAVO Directory Search Results

ID:: ivo://pds-ppi/radiojove_k4led_sdrrcpraw/ppi/epn_core
Title:: Radio JOVE Station K4LED SDRRCP Raw Data Collection
Short Name:: radiojove_k4led_
Date:: 25 Apr 2025 02:00:58
Publisher:: Planetary Data System
Description:: Radio JOVE Station K4LED SDRRCP Raw data from radio astronomy observations

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.

ID:: ivo://idoc/medoc/gaia_dem/q/epn_core
Title:: SDO GAIA-DEM
Short Name:: gaia_dem.epn_cor
Date:: 28 Apr 2025 03:12:17
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://vopdc.obspm/lerma/simrepo
Title:: SimDAL Repository
Short Name:: SimDAL Repo
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - LERMA
Description:: The SimDAL repository hosts numerical projects descriptions as standard XML documents following the Simulation Data Model serialization xsd. It allows clients to search (fulltext) for simulation projects or associated protocols of interest and get URIs towards other SimDAL components: SimDAL Search and SimDAL Data Access.

ID:: ivo://vopdc.obspm/imcce/skybot
Title:: Sky Body Tracker
Short Name:: SkyBoT
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - IMCCE
Description:: SkyBoT is a VO service which allows to seek and identify solar system objects (planet, satellites, asteroids, comets) in any field of view at a given epoch (cone-search method). It provides also a solar system object name resolver which convert the name or the designation of solar system objects into their celestial coordinates at a given epoch (resolver method). The SkyBoT service are available through a Web interface and a Web service (SOAP+WSDL+HTTP) which implements the IVOA Simple Cone-Search protocol.

ID:: ivo://vopdc.obspm/imcce/skybot/cea
Title:: Sky Body Tracker - Remote application
Short Name:: SkyBoT
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - IMCCE
Description:: SkyBoT is a VO service which allows to seek and identify solar system objects (planet, satellites, asteroids, comets) in any field of view at a given epoch (cone-search method). It provides also a solar system object name resolver which convert the name or the designation of solar system objects into their celestial coordinates at a given epoch (resolver method). The SkyBoT service are available through a Web interface and a Web service (SOAP+WSDL+HTTP) which implements the IVOA Simple Cone-Search protocol.

ID:: ivo://konkoly.hu/sbnaf/q/collection
Title:: Small Bodies Near and Far
Date:: 06 Sep 2023 06:07:48
Publisher:: Konkoly Observatory
Description:: SBNAF public database of thermal infrared observations of small bodies in the solar system. Our database collects thermal emission measurements of small Solar Systems targets that are otherwise available in scattered sources and gives a complete description of the data, with all information necessary to perform direct scientific calculations and without the need to access additional, external resources. See the details here: https://ird.konkoly.hu/

ID:: ivo://bira-iasb/soir/soir_q/epn_core
Title:: SOIR
Short Name:: soir.epn_core
Date:: 08 Oct 2024 09:26:16
Publisher:: Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
Description:: Profiles of species in Venus atmosphere terminator. Data retrieved from calibrated spectra obtained with the SPICAV-SOIR instrument on board the Venus Express spacecraft. These spectra can be checked on the ESA PSA repository. See: A.C. Vandaele et al., Contribution from SOIR/VEX to the updated Venus International Reference Atmosphere (VIRA), Adv. Space Res. (2015), http://dx.doi.org/10.1016/j.asr:2015.08.012.

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