Voyager 2 Magnetometer Jupiter Resampled System III Coords 9.60 Second
Data Collection
Short Name:
VG2_MAG_S3_9_60
Date:
15 Dec 2022 19:29:18
Publisher:
Planetary Data System
Description:
This collection contains Voyager 2 Jupiter encounter magnetometer
data from the Low Field Magnetometer (LFM) resampled at a 9.6 second
sample rate from the 60 msec instrument sampling rate. Data coverage
begins in the solar wind and continues until at least the first
magnetopause crossing. The data are given inJovicentric System
III(1965) right handed coordinates. All magnetic field observations
are measured in nanoTesla. All of the magnetic field data are
calibrated.
Voyager 1 Magnetometer Jupiter Resampled System III Coords 48.0 Second
Data Collection
Short Name:
VG1_MAG_J_S3_48S
Date:
15 Dec 2022 19:29:02
Publisher:
Planetary Data System
Description:
This collection contians calibrated magnetic field data acquired by
the Voyager 1 Low Field Magnetometer (LFM) during the Jupiter
encounter. Coverage begins in the solar wind inbound to Jupiter and
continues past the last outbound bowshock crossing. The data are in
System III (1965) (SYS3) coordinates and have been averaged from the
9.6 second summary data to a 48 second sample rate. All magnetic field
measurements are given in nanoTesla (nT).
Voyager 1 Magnetometer Jupiter Spacecraft Field Data Collection
Short Name:
VG1_MAG_J_SC_FLD
Date:
15 Dec 2022 19:29:33
Publisher:
Planetary Data System
Description:
This collection contains the estimated spacecraft field in payload
coordinates for the the Voyager 1 MAG 1.92, 9.6, and 48.0 second
averaged magnetic field data in heliographic (RTN) and Jovigraphic
System III (SYS3) coordinates, from the Jupiter encounter period
(1979-02-26 to 1979-03-24).
Voyager 2 Magnetometer Jupiter Spacecraft Field Data Collection
Short Name:
VG2_MAG_J_SC_FLD
Date:
15 Dec 2022 19:29:13
Publisher:
Planetary Data System
Description:
This collection contains sensor offset values in S/C coordinates from
the Magnetometer on Voyager 2 from the Jupiter encounter. The data
contains 48 second res. offset data.
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.
Voyager PRA (Planetary Radio Astronomy) Datasets catalog. The dataset
are originally published by several data centers: NASA/PDS,
NASA/NSSDC, NASA/GSFC, Univ. Iowa and CNES/SERAD.
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.
VPDs and CMDs of Berkeley32, Berkeley98 and King23
Short Name:
J/AJ/161/102
Date:
21 Oct 2021
Publisher:
CDS
Description:
Using the photometric and kinematical data from Gaia Data Release 2, three old open clusters namely Berkeley32 (Be32), Berkeley98 (Be98), and King23 are investigated. The latter two of these clusters are poorly studied in the literature. The numbers of the most probable cluster members are 563, 260, and 114 for Be32, Be98, and King23, respectively, with membership probabilities higher than 80% and lying within the clusters limiting radii. Mean proper motions (PMs; {mu}_{alpha}_cos_{delta}_ and {mu}_{delta}_) of the clusters are determined as (-0.34{+/-}0.008, -1.60{+/-}0.006), (-1.34{+/-}0.007, -3.22{+/-}0.008), and (-0.46{+/-}0.009, -0.87{+/-}0.012)mas/yr. The errors mentioned in the PMs are the Gaussian fitting errors. The blue straggler stars (BSS) in all three old clusters were found to exhibit centralized radial distribution. The clusters' radii are determined as 9.4', 12.95', and 6.6' for Be32, Be98, and King23 using radial density profiles. Ages of the clusters determined by isochrone fitting are 4.90{+/-}0.22, 3.23{+/-}0.15, and 1.95{+/-}0.22Gyr. The errors given in the clusters ages are the internal errors. The mass function slopes are found to be flatter than Salpeter's value for all three clusters. All three clusters are found to be dynamically relaxed. Galactic orbits are derived for these clusters, which demonstrate that the studied clusters follow a circular path around the Galactic center.
