Monday 13 February 2023, by Baptiste Cecconi, Laura Debisschop
This collection supplements: Wu et al. (2023), What can be deduced from the High Frequency Limit of Saturn’s Kilometric Radiation. J. Geophys. Res., (Submitted)
Raw text files
The collection is composed of three text files containing the northern and southern High Frequency Limit (HFL) for the Saturn kilometric radiation (SKR) as observed in Cassini/RPWS/HFR data:
Reading the raw data
Python code to load the data:
from astropy.time import Time
from astropy.units import Unit
import numpy
with open("SKRHFLderived_time_Format_t1997_v0830.txt", 'r') as f:
t = f.readline()
t = numpy.array(t.split(), dtype=float)
t = Time('1997-01-01') + (t - 1) * Unit('d')
print(f'Time range: {t[0].iso} to {t[-1].iso}')
with open("SKRHFLderived_HFL_N_v0830.txt", 'r') as f:
n = f.readline()
n = numpy.array(n.split(), dtype=float) * Unit('kHz')
with open("SKRHFLderived_HFL_S_v0830.txt", 'r') as f:
s = f.readline()
s = numpy.array(s.split(), dtype=float) * Unit('kHz')
Time range : 2004-01-01 to 2017-09-15
Spectral range : 98.9 kHz to 1.29 MHz
Location: Saturn
Acknowledgements
BC was supported by PADC and EPN2024-RI. The Europlanet 2024 Research Infrastructure (EPN2024-RI) project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149.
References