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).
*** USET sunspot drawing *** The Uccle Solar Equatorial Table (USET)
facility at the Royal Observatory of Belgium has gathered an
uninterrupted series of sunspot drawings since year 1941. This
collection continues to be updated when weather permits. This table
provides information about these drawings.
*** USET Groups *** Values in the USET sunspot group catalog are
derived from the solar drawings obtained by the Uccle Solar Equatorial
Table (USET) facility that is located at the Royal Observatory of
Belgium. The USET sunspot group catalog covers 82 years of
observations in 2021, and is updated every day. A home-made software
(DigiSun) written in Python is used to derive quantities such as
location and areas from the sunspot drawings.
Cassini Scalar Helium MAG Calibrated Housekeeping ASCII Data
Collection
Short Name:
CO-MAG-SHHKA
Date:
01 Mar 2024 22:33:54
Publisher:
Planetary Data System
Description:
This collections contains Cassini scalar helium magnetometer (SHM)
housekeeping ASCII data collected between 1999-08-18T02:56:40.391 and
2005-06-08T15:14:44.057.
Cassini MAG Calibrated 1 Min. Avg. Data in RTN Coords. Collection
Short Name:
CO-MAG-1MRTN
Date:
01 Mar 2024 22:11:02
Publisher:
Planetary Data System
Description:
This collection contains Cassini magnetic-field 1 minute averages,
from the Cassini Fluxgate Magnetometer (FGM), in RTN coordinates. RTN
coordinates consist of R (radial component, Sun to the spacecraft), T
(tangential component, parallel to the Solar Equatorial plane and
perpendicular to R), and N (normal component, completes right handed
set).
Cassini MAG Calibrated 1 Min. Avg. Data in KSO Coords. Collection
Short Name:
CO-MAG-1MKSO
Date:
01 Mar 2024 22:10:29
Publisher:
Planetary Data System
Description:
This collection contains Cassini magnetic-field 1 minute averages in
KSO coordinates, from the Fluxgate Magnetometer (FGM) instrument. KSO
coordinates consist of X (Saturn to Sun), Z (parallel to Saturn's
orbital plane upward normal), and Y (completes the right handed set).
Cassini MAG Calibrated 1 Min. Avg. Data in KSM Coords. Collection
Short Name:
CO-MAG-1MKSM
Date:
01 Mar 2024 22:05:18
Publisher:
Planetary Data System
Description:
This collection contains Cassini magnetic-field 1 minute averages in
KSM coordinates, from the Fluxgate Magnetometer (FGM) instrument. KSM
coordinates consist of X (Saturn to Sun), Z (X-Z plane contains
Saturn's centered magnetic dipole axis, M), and Y (completes right
handed set)
Cassini MAG Calibrated 1 Min. Avg. Data in KRTP Coords. Collection
Short Name:
CO-MAG-1MKRTP
Date:
01 Mar 2024 22:04:43
Publisher:
Planetary Data System
Description:
This collection contains Cassini magnetic-field 1 minute averages in
KRTP coordinates, from the Fluxgate Magnetometer (FGM) instrument.
KRTP coordinates are the standard right-handed spherical triad: R
(Saturn to spacecraft), Phi (parallel to Saturn's equator), and Theta
(completes right handed set).
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.
The Visual and Infrared Mapping Spectrometer (VIMS) instrument
onboard the Cassini spacecraft observed the system of Saturn,
acquiring spectral cubes in the range 0.4-5.2 microns. This service
focuses on Saturn satellites, and provides access to calibrated and
ancillary data, computed as described here:
https://vims.univ-nantes.fr/info/isis-calibration. It also provides
direct links to a larger web site with previews.
<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.
*** 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.
Voyager 2 Plasma Wave Science, Raw Waveforms, Entire Mission
Collection
Short Name:
VG2-PWS-WF
Date:
09 Nov 2023 17:33:51
Publisher:
Planetary Data System
Description:
This collection contains Voyager 2 Plasma Wave Spectrometer (PWS) raw
waveform data and documentation for all available telemetry frames
from (SCET) 1979-04-28T07:59:16.710Z through 2006-03-07T08:48:04.778Z.
The Voyager 1 PWS Electric Waveforms Data Collections contains raw
full resolution waveform data consisting of electric field waveform
samples from the Voyager 1 Plasma Wave Science waveform receiver
obtained during the entire mission.
Planetary Atmospheres Research Unit - Royal Belgian Institute for
Space Aeronomy
Description:
Profiles of pressure, temperature and species of the Martian
atmosphere simulated with the GEM-Mars general circulation model. See
for the main model descritpion Neary, L., et al. 2018. The GEM-Mars
general circulation model for Mars: Description and evaluation. Icarus
300, 458-476. https://doi.org/10.1016/j.icarus.2017.09.028. See for
the chemistry description Dearden, F. et al., 2019, Mars atmospheric
chemistry simulations with the GEM-Mars general circulation model,
Icarus, 326, 197-224, https://doi.org/10.1016/j.icarus.2019.02.030.
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.
Planetary Atmospheres Research Unit - Royal Belgian Institute for
Space Aeronomy
Description:
Profiles of pressure, temperature and species of the Martian
atmosphere derived from measurements of the NOMAD instrument on board
ESA's Trace Gas Orbiter. See paper
https://doi.org/10.1007/s11214-018-0517-2
Main characteristics of Solar System planets. Data are included in
the table, which includes non-standard EPN-TAP parameters. Data are
retrieved from Archinal et al 2018 (IAU report 2015,
2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical
quantities, 2000asqu.book.....C) [masses, heliocentric distances, and
rotation periods].
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/
MAG instrument raw status information, temperatures, voltage, command
status counts as well as low-resolution (14-bit) 3-axis magnetic field
samples as recorded by A/D converters integral to the Low Voltage
Power Supply (LVPS).
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
MESSENGER MAG Raw Science Header Information Data Collection
Short Name:
MESS-RAW-SHD
Date:
03 Feb 2023 20:18:09
Publisher:
Planetary Data System
Description:
Captures the instrument state (health and mode) as reported by the
science packet. This information only changes on packet boundaries so
it is kept in a separate EDR, minimizing repetition of information.
Each row in the Science Header EDR corresponds to the information
extracted from one science packet.
A cumulative file for the entire mission. The purpose of the file is
to keep a time log of bursts recorded by the instrument, as well as
the number of burst packets recorded for each Burst EDR.
Contains alternating current (AC) level values at the commanded
sample rate. To conserve telemetry the vector sampling will usually be
less than the maximum rate, 20 sample/s. To provide a record of the
amplitude of fluctuations for frequencies higher than 1 Hz, an AC
amplitude is calculated from the internally sampled 20/s data for the
sensor axis commanded as the AC_AXIS. Thus, in addition to the vector
samples data, a 1 Hz to 10 Hz bandpass average amplitude is evaluated
for the commanded sensor axis, selected by command, and recorded as a
log AC value with a 4-bit mantissa of the four most significant
non-zero bits and a 4-bit power of two exponent of the 4th (least
significant) bit of the mantissa. This is called the logAC value. It
is created once per second and saved for telemetry at that rate or at
the commanded science rate, whichever is less frequent.
MESSENGER MAG Low-Rate Header Information Data Collection
Short Name:
MESS-RAW-LHD
Date:
03 Feb 2023 20:17:27
Publisher:
Planetary Data System
Description:
MAG instrument state (health and mode) as reported by the LRHK
packet. This changes only on packet boundaries so it is kept in a
separate EDR, minimizing repetition of information. Each row in the
LHRK Header EDR corresponds to information extracted from one LHRK
packet.
MESSENGER MAG Low-Rate Housekeeping Information Data Collection
Short Name:
MESS-RAW-LHK
Date:
03 Feb 2023 20:17:11
Publisher:
Planetary Data System
Description:
This collection contains tables of instrument state as reported by
the MAG Low-Rate Housekeeping (LRHK) packet. It includes the 3-axis
field values (received from the filter and subsampling logic) and the
corresponding AC values.
This collection contains snapshots of MAG vector samples, or burst
sampling, over a time span of 8 minutes, at a rate of 20 samples per
second for a total of 9600 vector samples. The burst data give
information about waves and turbulent phenomena expected to occur at
the magnetospheric boundaries and elsewhere in association with pickup
processes of volatile species as they are photo-ionized. Typically one
burst period will be recorded every day of orbit operations.
The spacecraft potential based on all 4 sub-cycles and from both
booms merged to one time series. Note that data values of '-nan' can
be treated as equivalent to 'nan'.
MESSENGER MAG Calibrated Alternating Current Data Collection
Short Name:
MESS-MAG-CAL-LAC
Date:
06 Jan 2023 00:36:31
Publisher:
Planetary Data System
Description:
Ancillary MAG data containing calibrated alternating current (AC)
values of the average output amplitude a 1-to-10 Hz bandpass filter
for a single magnetometer axis selected by command.
MESSENGER MAG Calibrated RTN Coordinates Science Data Collection
Short Name:
MESS-MAG-RTN
Date:
06 Jan 2023 00:04:11
Publisher:
Planetary Data System
Description:
Calibrated 3-axis magnetic field samples in Radial-Tangential-Normal
(RTN) coordinates. The spacecraft position is given by the radial
distance from Sun center, northward latitude above the instantaneous
ecliptic plane, and azimuth angle of the spacecraft in the
instantaneous ecliptic plane with respect to the Earth-Sun line,
positive in direction of the Earth's orbital motion. The data are
tagged with latency corrected UTC and MET time stamps. The RTN CDR is
derived from the Science EDR.
MESSENGER MAG Time-Averaged Calibrated MSO Coordinates Science Data
Collection
Short Name:
MESS-MAG-MSO-AVG
Date:
06 Jan 2023 00:01:33
Publisher:
Planetary Data System
Description:
Time-averaged spacecraft position and calibrated 3-axis magnetic
field samples in Mercury Solar Orbital (MSO) coordinates. The data are
tagged with latency corrected UTC and MET time stamps at the center of
each interval. The MSO RDR is derived from the Science CDR for this
coordinate system with time averages computed within 1, 5, 10, and 60
s intervals.
MESSENGER MAG Time-Averaged Calibrated J2000 Coordinates Science Data
Collection
Short Name:
MESS-MAG-J2k-AVG
Date:
27 Dec 2022 02:13:02
Publisher:
Planetary Data System
Description:
Time-averaged spacecraft position and calibrated 3-axis magnetic
field samples in J2000 coordinates. The data are tagged with latency
corrected UTC and MET time stamps at the center of each interval. The
J2K RDR is derived from the Science CDR for this coordinate system
with time averages computed within 1, 5, 10, and 60 s intervals.
MESSENGER MAG Time-Averaged Calibrated Spacecraft Coordinates Science
Data Collection
Short Name:
MESS-MAG-SC-AVG
Date:
16 Dec 2022 17:31:44
Publisher:
Planetary Data System
Description:
Time-averaged calibrated 3-axis magnetic field samples in sensor and
spacecraft coordinates. The data are tagged with latency corrected UTC
and MET time stamps at the center of each interval. The SC RDR is
derived from the Science CDR for this coordinate system with time
averages computed within 1 s intervals.
Cassini RPWS Electron Densities from Upper Hybrid and Plasma Wave
Frequencies
Short Name:
CO-RPWS-ELC-DEN
Date:
16 Dec 2022 17:29:24
Publisher:
Planetary Data System
Description:
This collection provides electron number density values derived from
features observed in plasma wave data obtained by the Cassini Radio
and Plasma Wave Science (RPWS) instruments, along with observed or
derived characteristic frequencies, and useful positional parameters
for the spacecraft and related bodies. When present, frequency values
of narrowband emissions at the upper hybrid resonance were digitized
and combined with measured or model magnetic field to derive electron
number density. At other times, features such as the upper cutoff in
auroral hiss or electron plasma oscillations were used to determine
the plasma frequency and electron density.
MESSENGER MAG Calibrated J2000 Coordinates Science Data Collection
Short Name:
MESS-MAG-J2k
Date:
16 Dec 2022 17:28:24
Publisher:
Planetary Data System
Description:
Spacecraft position and calibrated 3-axis magnetic field samples in
J2000 coordinates. The data are tagged with latency corrected UTC and
MET time stamps. The J2K CDR is derived from the Science EDR.
MESSENGER MAG Calibrated Spacecraft Coordinates Science Data
Collection
Short Name:
MESS-MAG-SC
Date:
16 Dec 2022 17:23:28
Publisher:
Planetary Data System
Description:
Calibrated 3-axis magnetic field samples in sensor and spacecraft
coordinates. The data are tagged with latency corrected UTC and MET
time stamps. The SC CDR is derived from the Science EDR.
Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Electron
Spectrometer Data Collection
Short Name:
CO-CAPS-ELS
Date:
16 Dec 2022 17:19:17
Publisher:
Planetary Data System
Description:
This collection consists of all of the calibrated electron
spectrometer data from the Cassini Plasma Spectrometer (CAPS) on-board
the Cassini spacecraft during the entire Cassini mission.
MESSENGER MAG Time-Averaged Calibrated RTN Coordinates Science Data
Collection
Short Name:
MESS-MAG-RTN-AVG
Date:
16 Dec 2022 17:17:45
Publisher:
Planetary Data System
Description:
Time-averaged spacecraft position and calibrated 3-axis magnetic
field samples in Radial-Tangential-Normal (RTN) coordinates. The
spacecraft postion is given by the radial distance from Sun center,
northward latitude above the instantaneous ecliptic plane, and azimuth
angle of the spacecraft in the instantaneous ecliptic plane with
respect to the Earth-Sun line, positive in direction of the Earth's
orbital motion. The data are tagged with latency corrected UTC and MET
time stamps at the center of each interval. The RTN RDR is derived
from the Science CDR for this coordinate system with time averages
computed within 1, 5, 10, and 60 s intervals.
MESSENGER MAG Time-Averaged Calibrated MBF Coordinates Science Data
Collection
Short Name:
MESS-MAG-MBF-AVG
Date:
16 Dec 2022 17:16:54
Publisher:
Planetary Data System
Description:
Time-averaged spacecraft position and calibrated 3-axis magnetic
field samples in Mercury Body Fixed (MBF) coordinates. The data are
tagged with latency corrected UTC and MET time stamps at the center of
each interval. The MBF CDR is derived from the Science CDR for this
coordinate system with time averages computed within 1, 5, 10, and 60
s intervals.
Cassini-Huygens Plasma Spectrometer (CAPS) Calibrated Ion Mass
Spectrometer 'Time Of Flight' Straight Through Data Collection
Short Name:
CO-CAPS-TOFST
Date:
15 Dec 2022 19:30:57
Publisher:
Planetary Data System
Description:
This collection consists of all of the calibrated ion mass
spectrometer 'time of flight' straight through data from the Cassini
Plasma Spectrometer (CAPS) on-board the Cassini spacecraft during the
entire Cassini mission.
MESSENGER MAG Calibrated MBF Coordiantes Science Data Collection
Short Name:
MESS-MAG-MBF
Date:
15 Dec 2022 19:30:45
Publisher:
Planetary Data System
Description:
Spacecraft position and calibrated 3-axis magnetic field samples in
Mercury body fixed coordinates. The data are tagged with latency
corrected UTC and MET time stamps. The MBF CDR is derived from the
Science EDR.