Cover: Advanced Visible and Near Infrared Radiometer (AVNIR) observations of Mount Etna's aerosol plume

1998 ◽  
Vol 19 (15) ◽  
pp. 2823-2828 ◽  
Author(s):  
C. OPPENHEIMER P. FRANCIS I. M. WATSON
2021 ◽  
Vol 13 (7) ◽  
pp. 1399
Author(s):  
Quang Nguyen Hao ◽  
Satoshi Takewaka

In this study, we analyze the influence of the Great East Japan Earthquake, which occurred on 11 March 2011, on the shoreline of the northern Ibaraki Coast. After the earthquake, the area experienced subsidence of approximately 0.4 m. Shoreline changes at eight sandy beaches along the coast are estimated using various satellite images, including the ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer), ALOS AVNIR-2 (Advanced Land Observing Satellite, Advanced Visible and Near-infrared Radiometer type 2), and Sentinel-2 (a multispectral sensor). Before the earthquake (for the period March 2001–January 2011), even though fluctuations in the shoreline position were observed, shorelines were quite stable, with the averaged change rates in the range of ±1.5 m/year. The shoreline suddenly retreated due to the earthquake by 20–40 m. Generally, the amount of retreat shows a strong correlation with the amount of land subsidence caused by the earthquake, and a moderate correlation with tsunami run-up height. The ground started to uplift gradually after the sudden subsidence, and shoreline positions advanced accordingly. The recovery speed of the beaches varied from +2.6 m/year to +6.6 m/year, depending on the beach conditions.


1997 ◽  
Vol 12 (4) ◽  
pp. 21-25 ◽  
Author(s):  
Masanobu Shimada ◽  
Hiromi Oaku ◽  
Hiroyuki Oguma ◽  
Yuji Miyachi ◽  
Robert Green

1997 ◽  
Author(s):  
Kiyonari Fukue ◽  
Tamotsu Igarashi ◽  
Yuji Osawa ◽  
Haruhisa Shimoda ◽  
Ryuji Matsuoka ◽  
...  

1995 ◽  
Author(s):  
Yoshifumi Yasuoka ◽  
Masao Naka ◽  
Yuji Miyachi

2020 ◽  
Vol 12 (3) ◽  
pp. 427 ◽  
Author(s):  
Satoshi Tsuchida ◽  
Hirokazu Yamamoto ◽  
Toru Kouyama ◽  
Kenta Obata ◽  
Fumihiro Sakuma ◽  
...  

The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) onboard Terra platform, which was launched in 1999, has three separate subsystems: a visible and near-infrared (VNIR) radiometer, a shortwave-infrared radiometer, and a thermal-infrared radiometer. The ASTER VNIR bands have been radiometrically corrected for approximately 14 years by the sensor degradation curves estimated from the onboard calibrator according to the original calibration plan. However, this calibration by the onboard calibrator encountered a problem; specifically, it is inconsistent with the results of vicarious calibration and cross calibration. Therefore, the ASTER VNIR processing was applied by the radiometric degradation curves calculated from the results of three calibration approaches, i.e., the onboard calibrator, the vicarious calibration, and the cross calibration since February 2014. Even though the current degradation curves were revised, the inter-band and lunar calibrations show some inconsistencies owing to the different traceability in the bands by different calibration approaches. In this study, the current degradation curves and their problems are explained, and the new curves that are derived from the vicarious calibration with lunar calibration are discussed. The new degradation curves that have the same traceability in the bands will be used for future ASTER VNIR processing.


Sign in / Sign up

Export Citation Format

Share Document