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107 results for “Juno”
Juno Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic Inertial, and Solar Ecliptic Coordinates, HelioWeb, Daily Data
Heliocentric trajectories for Juno in Heliographic, HG, Heliographic Inertial, HGI, and Solar Ecliptic, SE, Coordinates The original trajectory data are taken from http://ssd.jpl.nasa.gov/horizons.cgi where users can find many more objects. In the case of orbit data for planets, the orbit data can be used as a proxy for spacecraft ephemeris that are in orbit about the planets. On a heliospheric scale, differences between the planet orbital tarjectory and that of the spacecraft are very small. For instance, the heliocentric longitudes differ by only 0.25° for a spacecraft stationed near the L1 Lagrange point at approximately 100 Earth radii upstream of the Earth. The production of the HG, HGI, and SE trajectory data requires a values for the "Equinox Epoch", which is defined as the epoch time when the direction from the Earth to the sun at the time of the vernal equinox when the sun seems to cross equatorial plane of the Earth from below. This direction is called the First Point of Aries, FPA and it is not a fixed direction but drifts by about 1.4° per century or 50.26" per year. In addition, there are tiny irregularities in FPA drift that are on the order of 1" per year or less. The Equinox Epoch can be determined by using a variety of methods for calculating the instantaneous FPA longitudinal direction and whether the tiny irregularities have been smoothed or averaged out. Four methods for determining the Equinox Epoch are in common usage: +---------------------------------------------------------------------+ Method Name FPA Longitude Definition --------------------------------------------------------------------- B1950.0 the actual FPA at 22:09 UT on December 31, 1949 J2000.0 the smoothed FPA at 12:00 UT on January 1, 2000 True of Date the actual FPA at 00:00 UT on the date of interest Mean of Date the smoothed FPA at 00:00 UT on the date of interest +---------------------------------------------------------------------+ The heliocentric trajectory data included in this data product have been calculated by using the Equinox Epoch: defined via the "Mean of Date" method. More precise coordinates, and some planet-centered coordinates, are found in the "traj" subdirectories of spacecraft specific directories at https://spdf.gsfc.nasa.gov/pub/data/ and http://ssd.jpl.nasa.gov/horizons.cgi.
Comprehensive analysis of small RNAs reveals insight into the tolerance of Ziyang xiangcheng (Citrus junos Sieb. ex Tanaka) to alkaline stress
GEO Series GSE115049. Citrus trifoliata; Citrus junos. 20 samples. Type: Non-coding RNA profiling by high throughput sequencing.
Comprehensive analysis of transcriptomes reveals insight into the tolerance of Ziyang xiangcheng (Citrus junos Sieb. ex Tanaka) to alkaline stress
GEO Series GSE115048. Citrus trifoliata; Citrus junos. 18 samples. Type: Expression profiling by high throughput sequencing.
Comprehensive analysis of transcriptomes and small RNAs reveals insight into the tolerance of Ziyang xiangcheng (Citrus junos Sieb. ex Tanaka) to alkaline stress
GEO Series GSE115050. Citrus trifoliata; Citrus junos. 38 samples. Type: Expression profiling by high throughput sequencing; Non-coding RNA profiling by high throughput sequencing.
JUNO J/SW JOVIAN AURORAL DISTRIBUTION CALIBRATED V1.0
This data set consists of all of the calibrated data collected by the JADE (Jovian Auroral Plasma Distributions Experiment) on-board the Juno spacecraft.
JUNO JUPITER MWR REDUCED DATA RECORDS V2.0
The Juno MWR RDR data sets will ultimately include all calibrated MWR science data records for the entire Juno mission. The set in this volume will contain only those data obtained during the orbital phase of the Juno mission, when this phase of the mission is completed. The RDR science records have a one-to-one correspondence with the EDR records.
JUNO MWR CRUISE/SKY RDR DATA RECORDS V3.0
The Juno MWR RDR data set will ultimately include all calibrated MWR science data for the entire Juno mission. This volume will contain only those data obtained through the cruise phase of the Juno mission, when this phase of the mission is completed. The objective for these data is to provide calibration for the MWR instrument; however, it is anticipated that they may someday be useful for astrophysics. This volume consists of calibrated data records, each of which contains all instrumental data required for further processing. The RDR records have a one-to-one correspondence with the EDR records.
JUNO OUTER CRUISE RAW GRAVITY SCIENCE 1 V1.0
This data set contains archival raw, partially processed, and ancillary/supporting gravity science data acquired during the Juno outer cruise between the October 2013 Earth Flyby and July 2016 Jupiter Orbit Insertion. The radio observations were carried out using the Juno spacecraft and Earth-based receiving stations of the NASA Deep Space Network (DSN). The data set was designed primarily to support testing and calibration of Juno's Gravity Science instrument. Of most interest are likely to be the Orbit Data Files in the ODF directory, which provided the raw input to gravity investigations, as well as the ionospheric an tropospheric media calibration files in the ION and TRO directories, respectively.
JUNO FGM CALIBRATED DATA SW V1.0
Abstract ======== This data set consists of the Juno FGM calibrated observations. The FGM sensor block uses two miniature ring-core fluxgate sensors to measure the magnetic field in three components of the vector field There are multiple FGM data products to accomodate different coordinate systems.
JUNO MOON JIRAM REDUCED DATA RECORD V3.0
This dataset contains the scientific telemetry produced by the JIRAM instrument , together with geometric information computed on ground to locate observations in space and time.
JUNO SW JOVIAN AURORAL DISTRIBUTION UNCALIBRATED V1.0
This data set consists of all of the uncalibrated data collected by the JADE (Jovian Auroral Plasma Distributions Experiment) on-board the Juno spacecraft. For more information about the instrument and data sets, see [MCCOMAS2013] and [WILSON2014].
JUNO JUPITER JIRAM REDUCED DATA RECORD V1.0
This dataset contains the scientific telemetry produced by the JIRAM instrument , together with geometric information computed on ground to locate observations in space and time.
JUNO JUPITER UVS 3 REDUCED DATA RECORD V1.0
The Juno Ultraviolet Spectrograph (UVS) CODMAC Level 3 Reduced Data Record is a collection of the far ultraviolet photon detections obtained by the UVS instrument, corrected for instrumental effects, radiometrically calibrated, and correlated with the auxiliary information needed to locate the observations in space and time. These data are organized, in a manner very similar to the RDR product files from which they are derived, into extensions within files formatted according to the Flexible Image Transport System (FITS) standard, version 2.1b. The UVS RDR archive enables reprocessing of the corrected and calibrated science data into far ultraviolet map products as map processing routines improve. Investigators interested in applying advanced mapping methods or needing to understand the properties of the corrected and calibrated data will find the RDR products useful. Many investigators, however, will be interested in using the UVS CODMAC Level 5 far ultraviolet map products directly.
JUNO JUPITER UVS 2 EXPERIMENT DATA RECORD V1.0
The Juno Ultraviolet Spectrograph (UVS) CODMAC Level 2 Experiment Data Record is a collection of the far ultraviolet photon detections obtained by the UVS instrument, in raw form. As such, it constitutes the permanent record of the raw UVS data. These data include both the instrument science and housekeeping data, organized into extensions within files formatted according to the Flexible Image Transport System (FITS) standard, version 2.1b. The UVS EDR archive enables reprocessing of the raw science data as radiometric and geometric calibration processing routines improve. Investigators interested in applying advanced calibration methods or needing to understand the properties of the raw data will find the EDR products useful. Most investigators, however, will be interested in using either the UVS data products contained in the CODMAC Level 3 Reduced Data Record, as radiometric and geometric calibration processing has already been done for these products, or the UVS CODMAC Level 5 far ultraviolet map products.
JUNO JUPITER JIRAM EXPERIMENT DATA RECORD V1.0
This dataset contains the scientific telemetry produced by the JIRAM instrument after editing for duplicated and corrupted packets, together with geometric information computed on ground to locate observations in space and time.
JUNO E/J/SS WAVES CALIBRATED SURVEY FULL RESOLUTION V1.0
The Juno Waves calibrated full resolution survey data set includes all low rate science electric spectral densities from 50Hz to 41MHz and magnetic spectral densities from 50Hz to 20kHz with complete sweeps at 30, 10 and 1 second intervals depending on the instrument mode. This is a complete full resolution data set containing all low rate science data received from Waves from launch until the end of mission including initial checkout, the Earth flyby, the Jupiter orbits and all cruise data. Data are acquired from the Waves Low Frequency Receiver (LFR) and High Frequency Receiver (HFR) and are processed into spectra on board. These data are presented as ASCII text spreadsheets for ease of use. This data set is intended to be the most comprehensive and complete data set included in the Juno Waves archive. Pre-rendered spectrograms generated from these data are included as well to lead the user to the particular data file(s) of interest. This data set should be among the first used of any in the Waves archive as it will lead one to the information required to locate more detailed products.
JUNO MWR CRUISE/SKY EDR DATA RECORDS V1.2
The Juno MWR EDR data set will ultimately include all uncalibrated MWR science data records for the entire Juno mission. This volume will contain only those data obtained through the cruise phase of the Juno mission, when this phase of the mission is completed. The objective for these data is to provide calibration for the MWR instrument; however, it is anticipated that they may someday be useful for astrophysics. This volume consists of reformatted and uncalibrated data records. The reformatting operation reassembles received instrument data packets into one-hour-long records of time-ordered data corresponding to 100-ms observations made by the MWR instrument. This data set is intended to preserve the full content of the uncalibrated instrument packets and is to be used only as a last resort. The level 3 MWR archived data are designed to be complete and more easily used.
JUNO SS FLUXGATE MAGNETOMETER CALIBRATED DATA V1.0
Abstract ======== This data set consists of the Juno FGM calibrated cruise observations. The FGM sensor block uses two miniature ring-core fluxgate sensors to measure the magnetic field in three components of the vector field. There are multiple FGM data products to accomodate different coordinate systems.
JUNO MWR CRUISE/SKY RDR DATA RECORDS V2.1
The Juno MWR RDR data set will ultimately include all calibrated MWR science data for the entire Juno mission. This volume will contain only those data obtained through the cruise phase of the Juno mission, when this phase of the mission is completed. The objective for these data is to provide calibration for the MWR instrument; however, it is anticipated that they may someday be useful for astrophysics. This volume consists of calibrated data records, each of which contains all instrumental data required for further processing. The RDR records have a one-to-one correspondence with the EDR records.
JUNO MWR CRUISE/SKY EDR DATA RECORDS V2.0
The Juno MWR EDR data set will ultimately include all uncalibrated MWR science data records for the entire Juno mission. This volume will contain only those data obtained through the cruise phase of the Juno mission, when this phase of the mission is completed. The objective for these data is to provide calibration for the MWR instrument; however, it is anticipated that they may someday be useful for astrophysics. This volume consists of reformatted and uncalibrated data records. The reformatting operation reassembles received instrument data packets into one-hour-long records of time-ordered data corresponding to 100-ms observations made by the MWR instrument. This data set is intended to preserve the full content of the uncalibrated instrument packets and is to be used only as a last resort. The level 3 MWR archived data are designed to be complete and more easily used.
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