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TESS Sector 61 observations include physical orbits 129 and 130 of the spacecraft around the Earth. Data collection was paused for a total of 0.63 days to download data. Data were downloaded approximately every seven days, once near apogee of each orbit and once near perigee. In total, there are 24.80 days of science data collected in Sector 61.
TESS Sector 62 observations include physical orbits 131 and 132 of the spacecraft around the Earth. Data collection was paused for a total of 0.63 days to download data. Data were downloaded approximately every seven days, once near apogee of each orbit and once near perigee. In total, there are 25.08 days of science data collected in Sector 62.
TESS Sector 58 observations include physical orbits 123 and 124 of the spacecraft around the Earth. Data collection was paused for a total of 0.63 days to download data. Data were downloaded approximately every seven days, once near apogee of each orbit and once near perigee. In total, there are 27.09 days of science data collected in Sector 58.
TESS Sector 60 observations include physical orbits 127 and 128 of the spacecraft around the Earth. Data collection was paused for a total of 0.63 days to download data. Data were downloaded approximately every seven days, once near apogee of each orbit and once near perigee. At TJD 2949.99, the spacecraft entered into safe mode, resulting in instrument turn-off until TJD 2955.04. There are no FFIs, target pixel file data, or light curve data during this time. During these times (as well as when the spacecraft is transmitting data to ground systems) the data and timestamps in target-pixel files and light curve files are set to NULL. One FFI from Camera 1 in orbit 127 was corrupted prior to downlink from the spacecraft and could not be recovered. The FFIINDEX number is 00738895 (timestamp 2022358084201), and no FFI file for Camera 1 was produced for this cadence. In total, there are 20.01 days of science data collected in Sector 60.
This paper describes the rationale and the protocol of the first component of the third simulation round of the Inter-Sectoral Impact Model Intercomparison Project (ISIMIP3a, http://www.isimip.org, last access: 2 November 2023) and the associated set of climate-related and direct human forcing data (CRF and DHF, respectively). The observation-based climate-related forcings for the first time include high-resolution observational climate forcings derived by orographic downscaling, monthly to hourly coastal water levels, and wind fields associated with historical tropical cyclones. The DHFs include land use patterns, population densities, information about water and agricultural management, and fishing intensities. The ISIMIP3a impact model simulations driven by these observation-based climate-related and direct human forcings are designed to test to what degree the impact models can explain observed changes in natural and human systems. In a second set of ISIMIP3a experiments the participating impact models are forced by the same DHFs but a counterfactual set of atmospheric forcings and coastal water levels where observed trends have been removed. These experiments are designed to allow for the attribution of observed changes in natural, human, and managed systems to climate change, rising CH 4 and CO 2 concentrations, and sea level rise according to the definition of the Working Group II contribution to the IPCC AR6.
Liquid sloshing in 45-deg sector compartmented cylindrical tanks
Northern quiet arcs in lower limit of latitude /us sector/ and its relation to magnetic storms & to the ring current magnetic field intensity
Frequency of appearance of noctilucent clouds over western sector of ussr
Imp-I satellite observations of interplanetary magnetic field revealing regular longitudinal sector structure in magnetic field rotating with Sun
Finite-amplitude free oscillations of inviscid incompressible fluid in cylindrical sector container
Digital system for accurate time sector division of spin stabilized vehicle as used on Pioneer space probes
Mapping interplanetary magnetic field by extrapolating satellite measurements, and sector evolution observations
Aspect system on Pioneer VI and VII INCORPORATES digital computer for accurate time sector division of spin stabilized vehicle
Interplanetary sector structure observed by IMP-I SATELLITE compared with photospheric magnetic field and plage structure observations
Evening sector polar magnetic substorm disturbance field morphology in transition region
Interplanetary magnetic field sector structure, noting Archimedes spiral directivity and 27 day recurrence period for pattern
Aerospace technology applications to civilian sector, noting spinoff and benefits
Interplanetary sector structure in rising portion of sunspot cycle