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1. CLIMSO coronagraphs at pic du midi de Bigorre
ID:
ivo://ov-gso/climso
Title:
CLIMSO coronagraphs at pic du midi de Bigorre
Short Name:
CLIMSO
Date:
23 Feb 2024 14:58:31
Publisher:
OVGSO
Description:
Pic du Midi de Bigorre in the French Pyrenees is the place where coronagraphic images were first realized, by Bernard Lyot in the 1930s. Since then, the solar instruments at Pic du Midi regularly provide images of the solar disc, solar prominences and solar corona.
2. Extrasolar Planets Encyclopaedia
ID:
ivo://vopdc.obspm/luth/exoplanet
Title:
Extrasolar Planets Encyclopaedia
Short Name:
ExoPlanet
Date:
10 Jan 2017
Publisher:
Paris Astronomical Data Centre - LUTH
Description:
VO-compliant and interactive encyclopaedia of extrasolar planets.
3. Illumination maps of 67P
ID:
ivo://cdpp/illu67p
Title:
Illumination maps of 67P
Short Name:
ILLU67P
Date:
02 Nov 2020 14:04:37
Publisher:
Centre de Données de la Physique des Plasmas(CDPP)
Description:
Illumination by the Sun of each face of the comet 67P/Churyumov-Gerasimenko based on the shape model CSHP_DV_130_01_LORES_OBJ.OBJ. The service provides the cosine between the normal of each face (in the same order as the faces defined in the shape model) and the Sun direction; both numerical values and images of the illumination are available. Each map is defined for a given position of the Sun in the frame of 67P (67P/C-G_CK). Longitude 0 is at the center of each map. The code is developed by A. Beth, Imperial College London, UK and the service is provided by CDPP (http://cdpp.eu). Acknowlegment: The illumination models have been developed at the Department of Physics at Imperial College London (UK) under the financial support of STFC grant of UK ST/N000692/1 and ESA contract 4000119035/16/ES/JD (Rosetta RPC-PIU). We would also like to warmly thank Bernhard Geiger (ESA) for his support in validating the 2D-illumination maps.
4. Nancay Decameter Array observation database
ID:
ivo://vopdc.obspm/usn/nda/epn
Title:
Nancay Decameter Array observation database
Short Name:
nda
Date:
25 Apr 2017 15:00:00
Publisher:
Paris Astronomical Data Centre - USN
Description:
Decametric radio observation from Nancay decameter array. The Nancay Decameter Array (NDA) at the Station de Radioastronomie de Nancay (SRN) is a phased array of 144 "Teepee" helicoidal antenna, half of which being Right Handed (RH) polarized and the other half being Left Handed (LH) polarized. Four receivers are currently connected to the NDA, sampling data in spectral ranges within 5 to 80 MHz.
5. Planetary and heliophysics plasma data at CDPP/AMDA
ID:
ivo://cdpp/amda
Title:
Planetary and heliophysics plasma data at CDPP/AMDA
Short Name:
AMDA
Date:
02 Nov 2020 14:03:51
Publisher:
CDPP
Description:
Planetary and heliophysics plasma data at CDPP/AMDA
6. VOEvent meteor shower service
ID:
ivo://padc.obspm.planeto/meteor_showers/q/epn_core
Title:
VOEvent meteor shower service
Short Name:
Meteor Showers
Date:
08 Mar 2023 13:09:31
Publisher:
Paris Astronomical Data Centre
Description:
The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravity of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82