EPNcore table of BASS2000, a Solar survey archive: Images, movies of
full Sun from groundbased instruments: Spectroheliographs of Meudon
and Coimbra, RadioHeliograph and Decametric Array of Nancay, CLIMSO,
USET
HST observations of planets, dwarf planets, and satellites, extracted
from the CADC database catalogue (with daily updates). Data are linked
to the CADC repository, with file names common to all HST archives.
Both calibrated and derived products are included. The main target is
identified. Physical ephemeris and thumbnails are provided when
available. Files and previews are not accessible during the
proprietary period.
Since 1973, the 18-cm lines of the OH radical have been
systematically observed in a number of comets with the Nançay radio
telescope. This allowed an evaluation of the cometary water production
rates and their evolution with time, as well as a study of several
physical processes: the excitation mechanisms of the OH radio lines,
the expansion of the cometary atmospheres, their anisotropy in
relation with non-gravitational forces, the Zeeman effect in relation
with the cometary magnetic field. The Nançay observations of 53
cometary apparitions between 1982 and 2009 are now organized in this
database.
"The growth of the Tharsis volcanic complex on Mars during
Noachian/Hesperian era induced a reorientation of the spin axis of the
planet (true polar wander). This service gives access to a map of Mars
topography before Tharsis formation (Early Noachian) and a map of Mars
topography before true polar wander (Late Noachian/Early Esperian),
from the model described in Bouley, S., Baratoux, D., Matsuyama, I. et
al. Late Tharsis formation and implications for early Mars. Nature
531, 344â347 (2016). https://doi.org/10.1038/nature17171 ."
"The data consists in topographic maps of synthetic 3D bodies
generated by a 3 parameters statistical model : the fractionally
integrated flux (FiF) (Lavallee, D., Lovejoy, S., Schertzer, D.,
Ladoy, P. (1993). Nonlinear variability and landscape topography:
analysis and simulation) adapted for spherical coordinates and
topography (Landais, F., Schmidt, F., and Lovejoy, S, (2018)
Topography of exoplanets, MNRAS). The 3 parameters are the following :
H: degree of smoothness; C1: degree of intermittency; alpha: degree of
multifractality; The service contains topographic maps (in Fits
format) and texture maps (in png format)."
Predictions of stellar occultations by the main planetary satellites
Short Name:
voccdb.epn_core
Date:
19 Apr 2024 14:16:01
Publisher:
Paris Astronomical Data Centre
Description:
The VOccDB database provides prediction and parameters of stellar
occultations by the main planetary satellites. Observations of a
stellar occultations help to better determine the size and the shape
of the occulting body, as well as its astrometric position at the
milli-arcsecond level precision. Only the main moons of giant planets
Jupiter, Saturn, Uranus and Neptune are considered in the event
prediction database. Predictions are provided over period 2023-2032,
up to visual magnitude 12 for the biggest satellites, and magnitude 14
for other satellites. For each stellar occultation event prediction,
the database provides circumstances and observational data, date and
timing of the occultation, star position and magnitude, excepted
duration, etc.
The database contains some outputs of the VCD for the scenarios : {1)
Standard cloud albedo Scenario, solar EUV average conditions ; 2)
Standard cloud albedo Scenario, solar EUV minimum conditions ; 3)
Standard cloud albedo Scenario, solar EUV maximum conditions ; 4) Low
cloud albedo Scenario, solar EUV average conditions ; 5) High cloud
albedo Scenario, solar EUV average conditions available}, at different
positions of latitude and longitude. These VCD outputs are provided as
Votables containing profiles of temperatures, pressures, density and
abundances of main species for altitudes between 0 and 349.5 km from
the surface.
Mars_dust provides a multiannual climatology of Martian airborne dust as measured by various space missions. The retrieved column dust optical depth is mapped for each Martian year and formatted as cubes with time in the 3rd dimension. Two versions are available: irregularly gridded maps, and regular maps produced by kriging. These latter maps are used as column-integrated dust scenarios in the Mars Climate Database (MCD v5). The detailed description of the methodology and dataset can be found in: Montabone et al (2015) Icarus 251, pp. 65-95https://doi.org/10.1016/j.icarus.2014.12.034 ; Montabone et al (2020) JGR-Planets https://doi.org/10.1029/2019JE006111
Paris Astronomical Data Centre - Constructor University
Description:
The Mars Crater Catalog by S.J. Robbins was generated from THEMIS
Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were
selected using 5 points along the rim. The table is statistically
complete to the diameter of ~1.0 km. The table contains morphologic
and morphometric data for craters with diameter larger than 3 km. The
Prometheus basin has been excluded from the Catalog due to technical
issues.
Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1)
Database Creation, Properties, and Parameters", S.J. Robbins and B.M.
Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI:
10.1029/2011JE003966
Paris Astronomical Data Centre - Constructor University
Description:
A catalogue of Mars craters by Lagain et al. (2020), extending the previous
catalogue from Robbins and Hynek (2012, DOI:10.1029/2011JE003966). 185 craters
were added by Lagain, the object IDs are compatible with the previous work.
Reference: "Impact cratering rate consistency test from ages of layered ejecta on Mars",
Lagain et al., Planetary and Space Science, v.180. (2020)
DOI: 10.1016/j.pss.2019.104755
Ulysses Jupiter Encounter Cospin Low Energy Telescope (LET) Flux Data
Collection
Short Name:
ULY-COSPIN-LET
Date:
04 Mar 2024 19:15:39
Publisher:
Planetary Data System
Description:
This file contains data submitted to the Planetary Data System (PDS)
by the Ulysses COSPIN investigators, for the Ulysses Jupiter
Encounter, 1992-01-25 to 1992-02-17 (days 25-48 inclusive). All data
on this volume are from the Low Energy Telescope (LET) detector.
Ulysses Jupiter Encounter Cospin Kiel Electron Telescope (KET) Raw
Data Collection
Short Name:
ULY-COSPIN-KET-R
Date:
04 Mar 2024 19:11:05
Publisher:
Planetary Data System
Description:
This file contains data submitted to the Planetary Data System (PDS)
by the Ulysses COSPIN investigators, for the Ulysses Jupiter
Encounter, 1992-01-24 to 1992-02-17 (days 25-48 inclusive). All data
on this volume are from the Kiel Electron Telescope (KET) detector.
Ulysses Jupiter Encounter Cospin Kiel Electron Telescope (KET)
Intensity Data Collection
Short Name:
ULY-COSPIN-KET-I
Date:
04 Mar 2024 19:10:39
Publisher:
Planetary Data System
Description:
This file contains data submitted to the Planetary Data System (PDS)
by the Ulysses COSPIN investigators, for the Ulysses Jupiter
Encounter, 1992-01-24 to 1992-02-17 (days 25-48 inclusive). All data
on this volume are from the Kiel Electron Telescope (KET) detector.
Ulysses Jupiter Encounter Cospin High Flux Telescope (HFT) Flux Data
Collection
Short Name:
ULY-COSPIN-HFT
Date:
04 Mar 2024 19:10:16
Publisher:
Planetary Data System
Description:
This file contains data submitted to the Planetary Data System (PDS)
by the Ulysses COSPIN investigators, for the Ulysses Jupiter
Encounter, 1992-01-25 to 1992-02-18 (days 25-48 inclusive). All data
on this volume are from the High Flux Telescope (HFT) detector.
Ulysses Jupiter Encounter Cospin High Energy Telescope (HET) Flux Data
Collection
Short Name:
ULY-COSPIN-HET
Date:
04 Mar 2024 19:09:00
Publisher:
Planetary Data System
Description:
This file contains data submitted to the Planetary Data System (PDS)
by the Ulysses COSPIN investigators, for the Ulysses Jupiter
Encounter, 1992-01-25 to 1992-02-17 (days 25-48 inclusive). All data
on this volume are from the High Energy Telescope (HET) detector.
Ulysses Jupiter Encounter Cospin Anisotropy Telescope (AT) Flux Data
Collection
Short Name:
ULY-COSPIN-AT
Date:
04 Mar 2024 19:08:32
Publisher:
Planetary Data System
Description:
This collection contains data submitted to the Planetary Data System
(PDS) by the Ulysses COSPIN investigators, for the Ulysses Jupiter
Encounter, 1992-01-25 to 1992-02-17 (days 25-48 inclusive).