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457 results for “voyager”
Data from: A voyage to Terra Australis: human-mediated dispersal of cats
Open the record for dataset details and reuse information.
Figures 8-9 from: Chatzimanolis S (2014) Darwin's legacy to rove beetles (Coleoptera, Staphylinidae): A new genus and a new species, including materials collected on the Beagle's voyage. ZooKeys 379: 29-41. https://doi.org/10.3897/zookeys.379.6624
Figures 8-9 - Aedeagus of Darwinilus sedarisi Chatzimanolis, sp. n. 8 Dorsal view 9 Lateral view.
Computer Simulation of Viking Voyages: Oseberg_March_2021
<p>Contains computer simulated routes of Viking voyages for the Oseberg, with wind data from March 2021. Divided by Route_Month_Year_RouteNumber_Date_Time.</p>
Computer Simulation of Viking Voyages: Oseberg_September_2005
<p>Contains computer simulated routes of Viking voyages for the Oseberg, with wind data from September 2005. Divided by Route_Month_Year_RouteNumber_Date_Time.</p>
Computer Simulation of Viking Voyages: Roar_Ege_December_2021
<p>Contains computer simulated routes of Viking voyages for the Roar Ege, with wind data from December 2021. Divided by Route_Month_Year_RouteNumber_Date_Time.</p>
Computer Simulation of Viking Voyages: Roar_Ege_September_2005
<p>Contains computer simulated routes of Viking voyages for the Roar Ege, with wind data from September 2005. Divided by Route_Month_Year_RouteNumber_Date_Time.</p>
A Feasibility Study of the Nativis Voyager® System in Patients With Recurrent Glioblastoma Multiforme (GBM) in Australia
ClinicalTrials.gov study NCT02507102. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Nativis Voyager for Newly Diagnosed GBM
ClinicalTrials.gov study NCT03276286. IPD Sharing: NO. Countries: 1. Publications: 0.
Valsartan Optimal Therapy Against Elevated Home Blood Pressure Research（VOYAGER）Study
ClinicalTrials.gov study NCT00460213. IPD Sharing: Not stated. Countries: 1. Publications: 0.
A Study Related to the VOYAGER PAD Trial to Learn More About the Target Population for Xarelto in French Patients
ClinicalTrials.gov study NCT04824729. IPD Sharing: NO. Countries: 1. Publications: 0.
Phase 2 Trial of Voyager V1 in Combination With Cemiplimab in Cancer Patients
ClinicalTrials.gov study NCT04291105. IPD Sharing: NO. Countries: 2. Publications: 0.
Voyager 1 Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic Inertial, and Solar Ecliptic Coordinates, HelioWeb, Daily Data
Heliocentric trajectories for Voyager 1 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.
Voyager 2 Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic Inertial, and Solar Ecliptic Coordinates, HelioWeb, Daily Data
Heliocentric trajectories for Voyager 2 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.
Guselkumab reduces disease- and mechanism-related biomarkers more than adalimumab in patients with psoriasis: a VOYAGE 1 substudy
GEO Series GSE252029. Homo sapiens. 181 samples. Type: Expression profiling by array.
FIGURE 6 in Additional notes on the publication of the Narrative, Zoology and Notes from a Journal of Research into the Natural History of the Voyage of H.M.S. Samarang and its consequences for the nomenclature of decapod crustaceans and other taxa
FIGURE 6. Advertisements that are bound at the end of copies of the first volume of the Narrative (Belcher 1847a): A, B, the first two pages of the 'first set' of advertisements; C, the second page of the 'second set' of advertisements.
FIGURE 5 in Additional notes on the publication of the Narrative, Zoology and Notes from a Journal of Research into the Natural History of the Voyage of H.M.S. Samarang and its consequences for the nomenclature of decapod crustaceans and other taxa
FIGURE 5. Title-page and frontispiece of the second volume of the Narrative (Belcher 1847b) which encompasses the Natural History (Adams 1847c).
FIGURE 3 in Additional notes on the publication of the Narrative, Zoology and Notes from a Journal of Research into the Natural History of the Voyage of H.M.S. Samarang and its consequences for the nomenclature of decapod crustaceans and other taxa
FIGURE 3. Extracts from the two volumes of The Samarang Scrap-Book which are held by the Dixson Library at the State Library of New South Wales, Australia. The volumes contain drawings made during the voyage of the Samarang, some of which are signed by Arthur Adams: A, the 'title-page' of the first volume (call no. DGA 39/vol. 1); B, a drawing of a spider from the second volume (call no. DGA 39/vol. 2); C, a close-up view of the drawing in B showing the signature of Arthur Adams. Images courtesy of the Dixson Library at the State Library of New South Wales.
FIGURE 2. Extracts from a in Additional notes on the publication of the Narrative, Zoology and Notes from a Journal of Research into the Natural History of the Voyage of H.M.S. Samarang and its consequences for the nomenclature of decapod crustaceans and other taxa
FIGURE 2. Extracts from a parliamentary report entitled "Collection during the voyages of H.M.S. Samarang" in which the correspondence of Adams and Belcher in relation to the funding of the plates of the Zoology by the British Government are reproduced (Anonymous 1848a: 229, 230).
Voyager I: Patient Discharge Using the AB5000 Portable Driver System
ClinicalTrials.gov study NCT00971776. IPD Sharing: Not stated. Countries: 0. Publications: 0.
VOYAGER 2 JUPITER MAGNETOMETER RESAMPLED DATA 1.92 SEC
This data set includes Voyager 2 Jupiter encounter magnetometer data that have been resampled at a 1.92 second sample rate. The data set is composed of 6 columns: 1) ctime - this column contains the data acquisition time. The time is always output in the ISO standard spacecraft event time format (yyyy-mm-dd-Thh:mm:ss.sss) but is stored internally in Cline time which is measured in seconds after 00:00:00.000 Jan 01, 1966, 2) br - this column contains the radial component of the magnetic field, 3) bphi - this column contains the phi component of the magnetic field, 4) btheta - this column contains the theta component of the magnetic field, 5) bmag - this column contains the magnitude of the magnetic field, 6) flag - a flag value that indicates either software error or spacecraft hardware interference reduced confidence in this record (flag value of 1 is bad , 0 is good or unchecked). All magnetic field observations are measured in nanoTeslas. The coordinate system for this dataset is Minus System III. All of the magnetic field data are calibrated (see the instrument calibration description for more details). The Jupiter System III coordinate system is defined in Dessler 1983 and the reference documents for this dataset are: Ness et al, 1979A Lepping et al, 1981 Connerney,Acuna,Ness, 1981 Behannon,Burlaga,Ness, 1981
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