7/7/2023 0 Comments Omniweb spacecraft data![]() UAE lunar rover will test 1st artificial intelligence on the moon with Canada Changing orbit to Deimos Sultan Al Neyadi to perform 1st spacewalk by an Arab astronaut this month UAE Mars orbiter creates stunning new map of the Red Planet Related: The UAE's Hope mission to Mars in photos The papers also highlighted the lower atmosphere and how it changes throughout the day, seasons, and year, the visual appearance of light and dark surfaces, the atmospheric phenomena including clouds, fog, dust, and water ice clouds, as well as the Sinuous Discrete Aurora. They also focused on the migrating thermal tides in the atmosphere, the Martian dayglow emissions, diurnal variations, the spatiotemporal structure of far ultraviolet Martian dayglow, combined analysis of hydrogen and oxygen emissions, various types of aurorae and many other phenomena on Mars. The papers included studies on the current state of the Martian atmosphere, the planet's climate, and various natural phenomena, such as dust storms, atmospheric waves and large-scale dynamics. The EMM science team was able to publish several papers covering key data and findings captured by the science instruments on the Hope Probe, including the Emirates Mars InfraRed Spectrometer (EMIRS), Emirates Mars Ultraviolet Spectrometer (EMUS) and the Emirates Exploration Imager (EXI). It has published 13 new papers through the American Geophysical Union's (AGU) Geophysical Research Letters (GRL), under a special issue titled "The First Results from the Emirates Mars Mission (EMM)." Since its entrance into space, the Hope Probe has made a significant contribution to the scientific community. The Hope Probe's contribution to the scientific community On top of this, images of the patchy discrete aurora, atomic hydrogen and Martian water-ice clouds have made the EMM the first mission to Mars to be able to characterize the daily variations of the atmosphere within and across the Martian seasons. The observation of both these two types of diffuse aurora, observed during intense solar storms and the discrete aurora, along with a third aurora, the proton aurora, has meant that our Hope Probe has managed to observe auroras on both nightside and dayside Mars. Between the three types of aurorae the Probe has captured, our spacecraft has even captured intricate imagery of the notoriously mysterious Sinuous Discrete Aurora. The images that the Hope Probe has been able to capture are not only visually stunning but have contributed massively to a further understanding of the Red Planet's atmosphere, while offering magnificent imagery of space that is testimony to the impressive technology our community has designed. Perhaps most notably, our Hope Probe has captured high-cadence images of Mars' aurora. VxO's have the options of identifying and/or otherwise exploiting these value-added interfaces in response to relevant user queries and of identifying and possibly retrieving the corresponding FTP-accessible ASCII files.Despite entering space only three years ago, our probe has already picked up an abundance of high-cadence imagery and data. For the latter two, filtering by any parameters in the records enables study of dependences of CCF's, means, etc. In addition, many data sets also have scatter plot, linear regression fitting and cross correlation coefficient (CCC) determination capabilities, while some have distribution function and statistics (means, medians, etc.) capabilities. These interfaces provide baseline functionalities of time span selection and subsetting by physical parameter, with plot, list and file creation options. FTPBrowser provides access to many tens of higher resolution heliospheric magnetic field, plasma and energetic particle data sets. Data have been uniformized in content, format and coordinate system usage. COHOWeb provides access to hourly resolution solar wind magnetic field and plasma data from each of many deep space spacecraft (Voyagers, Pioneers, Ulysses, Helios) and to the OMNI data near Earth. ![]() The spacecraft-specific 1-min data are also OMNIWeb- accessible. Very recently, OMNIWeb began providing access to 1-min and 5-min versions of OMNI data for 1995 to near-current, based on ACE, Wind and IMP 8 data shifted to the Earth's bow shock nose by a combination of minimum variance and cross product techniques applied to ~15-s magnetic field data. Cross-normalized data from each of many spacecraft are used. OMNIWeb provides access to hourly resolution near-Earth solar wind magnetic field and plasma data for 1963 to near-current.
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