#Offset explorer update#
#Offset explorer full#

Information by state, and world seismicity maps. Use real-time web services for your own applications. Get real-time earthquake notifications sent to you on your phone or by email, or subscribe to real-time feeds. Real-time Notifications, Feeds, and Web Services Analyze multidimensional metrics, whether built in to Dynatrace or ingested. Various output formats, and links to earthquake details. The Data explorer greatly enhances your abilities to query and chart metrics. View historic seismicity, find past earthquakes that meet your criteria. USGS and non-USGS collections of earthquake-related features and effects and shaking damage. Special Earthquakes, Earthquake Sequences, and Fault ZonesĬompilations of information about significant earthquakes, swarms or sequences, and fault zones of interest.

Largest earthquakes, significant events, lists and maps by magnitude, by year, or by location. Tap/click on 'gear icon' for options and settings. Photo by Peter Haeussler, USGS, November 9, 2002. (d) During clear or photometric nights in which MUSE science OBs are executed.Peter Haeussler prepares to measure the offset of a crevasse on the Canwell Glacier, Alaska, USA. (c) These single flat fields are taken automatically at hourly intervals during the night or when the change in temperature is above 0.3 degrees. Every 90 days we take 15 frames per lamp to obtain the Line Spread Function (LSF). (b) The default is to obtain five exposure per lamp for each of the Ne, Xe, and HgCd lamps. All other modes are calibrated if used during the night. (a) Every day we obtain flats and arcs as described below for mode WFM-NOAO-E. Wavelength solution, Dispersion characteristicsĪbsolute flux calibration. To help bring resources back into the countries most affected, shop local and support local businesses in your travels. You can also manually specify ROI values for X-Offset, Y-Offset, Width. Illumination correction, Tracing solution, Background light, Instrument throughput. Launch the Image Acquisition Explorer app and explore its capabilities.

#Offset explorer update#

Geometrical calibration: Multi-Pinhole mask with arc lamps Exciting update to our Offset library Side view of female explorer in outerwear standing near stone arch and taking selfie on. These are the main performed as part of the standard calibration plan. Starting P103 offers a 7.5x7.5 arcsec 2 LTAO corrected field of view sampled at 0.025'/pixel (NFM-AO). Since P101 MUSE offers the GLAO mode of the VLT Adaptive Optics Facility (AOF) via the GALACSI adaptive optics module, offering an AO corrected 1'x1' field of view with 0.2 arcseconds sampling (WFM-AO). Spatially, the instrument samples the sky with 0.2 arcseconds spatial pixels in the currently offered Wide Field Mode with natural seeing (WFM-noAO).

#Offset explorer full#

Spectrally the instrument samples almost the full optical domain with a mean resolution of 3000. It has a modular structure composed of 24 identical IFU modules that together sample, in Wide Field Mode (WFM), a near-contiguous 1 squared arcmin field of view. Share your favorite Ford Explorer ST photos as well as engage in discussions with fellow Ford Explorer ST owners on our message board. We offer one of the largest collection of Ford Explorer ST related news, gallery and technical articles. MUSE, the Multi- Unit Spectroscopic Explorer, is an Integral Field Spectrograph located at the Nasmyth B focus of Yepun, the VLT UT4 telescope. Ford Explorer ST Forum is the premier Ford Explorer ST community.