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LOFAR PL610 Station Data Product Specification Cover

Figures & Tables

Figure 1.

The Space Research Centre, PAS, LOFAR PL610 Station in Borówiec, Poland. (1) Container with electronic equipment; (2) Low Band Antenna Field;
(3) High Band Antenna Field (Pożoga et al., 2021)
The Space Research Centre, PAS, LOFAR PL610 Station in Borówiec, Poland. (1) Container with electronic equipment; (2) Low Band Antenna Field; (3) High Band Antenna Field (Pożoga et al., 2021)

Figure 2.

The Dst index for 9th of June, 2021
The Dst index for 9th of June, 2021

Figure 3.

The I Signal Intensity (top) and the S4 index for 300-second time window (bottom) plots of the recovery phase after the geomagnetic storm for CasA radio source
The I Signal Intensity (top) and the S4 index for 300-second time window (bottom) plots of the recovery phase after the geomagnetic storm for CasA radio source

Figure 4.

The Dst index for March 15th, 2022
The Dst index for March 15th, 2022

Figure 5.

The I Signal Intensity (top) and the S4 index for 300 second time window (bottom) plots of the recovery phase after the geomagnetic storm for the CasA radio source
The I Signal Intensity (top) and the S4 index for 300 second time window (bottom) plots of the recovery phase after the geomagnetic storm for the CasA radio source

The metadata of the standardized LOFAR PL610 data product

Name of the attributeAttribute description
StartTimetimestamp marking the beginning of the observation given in ISO 8601 datetime YYYY-MM-DDTHH:mm:ss(.SSSSSS) format
StopTimetimestamp marking the end of the observation given in ISO 8601 datetime YYYY-MM-DDTHH:mm:ss(.SSSSSS) format
Lanetechnical parameters defining which lane was used during measurements. It is a numerical value (e.g., 1, 2, 3 or 4)
Targetthe radio source used for the observations (e.g., CasA, TauA, CygA, VirA, Sun, Jupiter)
Digdirthe right ascension, declination, and epoch (J2000 for the available data)
Anadirthe right ascension, declination, and the epoch (J2000 for the available data) for HBA analogue beam forming
Bandthe bands on which the observations were carried out (e.g., 10_90, 110_190, 210_270) given in MHz
SoftRevSoftware Revision; it includes the name of the computer
Datatypethe type of the data
Observatorythe LOFAR station from which the observations were carried out. In the case of the described data sets – PL610 station
Bitmodesource data bit resolution 4/8/16 bits
FFTLengththe additional subband division using FFT (e.g. 1, 16). 1 – no division, spectral resolution: 195.0 kHz; 16 – spectrum resolution increase to 12.2 kHz
TimeLengththe time of the observation given in seconds [s] and multiplied by 100 Hz; the number of samples measured per second
SubbandNothe number of observed frequencies
dimensions(sizes)Time(TimeLength), Subband(SubbandNo)
variables(dimensions)the variables including Stokes parameters (I, U, V, Q) given as float32 variables: I(Subband,Time), U(Subband,Time), V(Subband,Time), Q(Subband,Time), N(Time) – int64 – the number of samples, and Subband – given as float32 Subband(Subband)
DOI: https://doi.org/10.2478/arsa-2024-0006 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
Language: English
Page range: 77 - 86
Submitted on: Dec 22, 2023
Accepted on: Sep 6, 2024
Published on: Oct 8, 2024
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2024 Helena CIECHOWSKA, Mariusz POŻOGA, Barbara MATYJASIAK, Łukasz TOMASIK, Thi PHUNG, Katarzyna BESER, Marcin GRZESIAK, Roman WRONOWSKI, Hanna ROTHKAEHL, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons Attribution 4.0 License.