18 datasets

NASA Earthdata CMR2018 · collection

All-sky images taken from the Cloud-Cam instrument on the RSV Aurora Australis during the K-Axis campaign between 22-Jan-2016 and 16-Feb-2016 [days 22 to 47]. Images were acquired at 1-minute cadence, and are presented as timelapse movies analysed for cloud fraction, and keograms (obtained by horizontally accumulating a vertical slice through the zenith pixel of each image).

NASA Earthdata CMR2015 · collection

These datasets were acquired in the 2010/2011 and 2012/2013 Summer seasons from a multi-rotor unmanned aircraft system (UAS), also known as OktoKopter. This research focuses on the development of novel remote sensing techniques to map the spatial variability of moss bed health. At each site we flew the OktoKopter with three sensors: 1) an RGB digital SLR camera resulting in ultra-high resolution a

NASA Earthdata CMR2008 · collection

All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders and TEAC recorder. The all-sky video data is recorded on VHS tapes with two copies, one for Polar Research Institute of China, and the other copy goes to National Institute of Polar Research, Japan, ac

NASA Earthdata CMR2004 · collection

All Sky Imager Systems (ASIS) are deployed at Casey, Davis, Macquarie island and Mawson. These systems are autonomous data collection systems which record All Sky Imager data during periods of darkness at the stations. The data are collected using a monochromatic video camera fitted with an Image Intensifer and a Fish eye lens. A filter (normally 558 nm) is also fitted to the cameras. (this can be

NASA Earthdata CMRcollection

Observation of auroral displays at the Italian Antarctica Station Mario Zucchelli located at Terra Nova Bay to investigate the physical processes responsible for magnetosphere-ionosphere coupling and energy relaxation.

NASA Earthdata CMRcollection

All-sky camera (Prede, Model PSV-100) was placed on the roof-top of Rabben Station in Ny-Alesund, Svalbard and acquires all-sky color images on a continuous operation basis with a time resolution of a 10 min interval since 6 March 2005.

NASA Earthdata CMRcollection

Optical observations of auroral displays are performed by a camera with a field of view of 180 degrees: the all-sky camera. A prototype camera has been delivered to the Argentinian base General Belgrano II.The present instrument has been equipped with a 512x382 CCD and a filter wheel housing three filters in order to provide spectral discrimination at 630.0 nm, 557.7 nm and 427.8 nm. The instrumen

NASA Earthdata CMRcollection

Auroral morphological, dynamical, and spectroscopic observations have been carried out at Syowa Station with various ground-based auroral optical instruments. Auroral observations have been carried out since the establishment of Syowa Station in 1957. Currently operated instruments are: All-sky monochromatic imager (ASI), All-sky TV camera (ATV), Multi-color meridian scanning photometer (SPM), and

NASA Earthdata CMRcollection

This is a Sino-Japan collaborative observation at Zhongshan Station, Antarctica, which commenced in March 1995 (Principal Investigators: Prof. Natsuo Sato, National Institute of Polar Research and Dr. Huigne Yang, Polar Research Institute of China). The observation system comprises a HARPICON (High-gain Avalanche Rushing Amorphous Photoconductor) TV camera fitted with a fish-eye lens. A HARPICON t

NASA Earthdata CMRcollection

All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders and TEAC recorder. The all-sky video data is recorded on VHS tapes with two copies, one for Polar Research Institute of China, and the other copy goes to National Institute of Polar Research, Japan, ac

NASA Earthdata CMRcollection

All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders and TEAC recorder. The all-sky video data is recorded on VHS tapes with two copies, one for Polar Research Institute of China, and the other copy goes to National Institute of Polar Research, Japan, ac

NASA Earthdata CMRText

All-sky TV camera is used to monitor aurora display nearly 180 degrees in filed of view, it consists of an all-sky camera,a control box, a timing generator, a time corrector, two HD-DVD recorders and a video output monitor. The all-sky video data is recorded on DVD-Rs with two copies, one for Polar Research Institute of China, and the other copy goes to National Institute of Polar Research, Japan,

NASA Earthdata CMRText

All-sky TV camera is to monitor auroral displays nearly 180 degrees in filed of view, it consists of all-sky camera, control box, timing generator, timer corrector, two VHS recorders, SVHS recorders and TEAC recorder. The all-sky video data is recorded on VHS tapes with two copies, one for Polar Research Institute of China, and the other copy goes to National Institute of Polar Research, Japan, ac

NASA Earthdata CMRcollection

All-sky Imager Observation at South Pole Station

NASA Earthdata CMRcollection

The Coupling, Energetics, and Dynamics of Atmospheric regions (CEDAR) is a program sponsored by the National Science Foundation (NSF) designed to enhance the capability of ground-based instruments to measure the upper atmosphere and to coordinate instrument and model data for the benefit of the scientific community. The CEDAR Data Base (formally the Incoherent Scatter Radar Data Base) is a coopera

NASA Earthdata CMRcollection

This is a Sino-Japan collaborative observation at Zhongshan, Antarctica, which commenced March 1998 (Principal Investigators: Prof. Natsuo Sato, National Institute of Polar Research and Dr. Huigen Yang, Polar Research Institute of China). The observation system comprises a CCD camera fitted with a fish-eye lens and an interference filter, which can be manually changed between the two target aurora

NASA Earthdata CMRcollection

The Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR) Data Base at NCAR/HAO holds data collected from airglow imagers and all-sky cameras. None of the imager data are in digital form in the CEDAR Data Base and must be obtained from the contact person. Video tapes from the imager at Millstone Hill are in the CEDAR Data Base. Other data are as follows: 1. Utah State University CCD im

NASA Earthdata CMRcollection

The location of the Belgrano Station in the auroral zone facilitates the observation of auroral activity and its correlation with other geophysical events. The data was acquired continuously through out the polar night.