The Dependence of Log Periodic Dipole Antenna (LPDA) and e-CALLISTO Software to Determine the Type of Solar Radio Burst (I -V)

Sabri, S. N. U.; Zainol, N. H.; Ali, M. O.; Shariff, N.N.M.; Hussien, NurulHazwani; Faid, M. S.; Hamidi, Zety Sharizat; Monstein, C.

doi:10.1109/icimsa.2016.7504039

Cited by 10 publications

(2 citation statements)

References 1 publication

Supporting

Mentioning

Contrasting

Order By: Relevance

“…As a result of the structure of the Sun, the solar bursts indicate the Sun is active. Depending on the factors involved, solar bursts can be classified into five types, from type I to type V [1]. Compared to other bursts, solar burst type III is the most common, mostly caused by solar flares.…”

Section: Introductionmentioning

confidence: 99%

Moderate Radio Flux Density of Single and Group III Bursts from AR2887 Active Region on 26th October 2021

Hamidi

Chen

Nurlisman

2022

J. Phys.: Conf. Ser.

View full text Add to dashboard Cite

The radio flux density is one of the most important parameters for predicting solar activity, such as solar flares and Coronal Mass Ejections. Compared to other burst types, solar burst type III (SRBT III) occurs most frequently due to solar flare phenomena. In the meter and decimetre wavelength range, gyro synchrotrons dominate, as do localized disturbances in the plasma frequencies caused by SRBT III. In this paper, we examine the most recent solar event that took place on 26th October 2021 in this gradual phase of the 25th solar cycle and can be detected from our site. In order to compare our results to other regions of the electromagnetic spectrum, we also used the data from the Solar Monitor and Space Weather Live website, where the data from NOAA and SDO/AIA were made publicly available. A wavelength of 10.7 cm corresponds to 101 solar flux units. Approximately 4.7 nT of interplanetary magnetic field exists and 1.7 nT in the northward direction. In the past 6 hours and 24 hours, flares of class C2 and M1 have been detected due to active region AR2887 generated by a 'beta-gamma' magnetic field.

show abstract

Section: Introductionmentioning

confidence: 99%

Moderate Radio Flux Density of Single and Group III Bursts from AR2887 Active Region on 26th October 2021

Hamidi

Chen

Nurlisman

2022

J. Phys.: Conf. Ser.

View full text Add to dashboard Cite

show abstract

“…Single large aperture concept and three substrate layers consisting of air between FR4 are utilized to obtain high gain. Measurement result shows that the proposed antenna indeed inherits high gain, up to 9.61 dBi, which might alsobe used to monitor solar activity [13,14], or even to collect solar RF energy.…”

Section: Introductionmentioning

confidence: 99%

Development of Large Aperture Microstrip Antenna for Radio Wave Energy Harvesting

Savitri¹,

Anwar²,

Amrullah³

et al. 2018

PIER Letters

View full text Add to dashboard Cite

Abstract-Radio wave energy harvesting has become one of the most fascinating fields of research, especially in developing antenna for its front end subsystem. This paper presents the development of a single large aperture antenna for energy harvesting system. Three substrate layers FR4-air-FR4 are employed to increase the antenna gain. Measurement result shows that the proposed antenna is able to obtain gain of about 9.61 dBi at 1.575 GHz (GPS L1 frequency), with low return loss of about −17.12 dB. The achieved bandwidth is about 128 MHz. The antenna characteristic is suitable for energy harvesting application.

show abstract

Investigation of Characteristics of Noise Storm Solar Burst Type I on 11th March 2013

Hamidi

Shariff

2018

Lecture Notes in Electrical Engineering

View full text Add to dashboard Cite

The Dependence of Log Periodic Dipole Antenna (LPDA) and e-CALLISTO Software to Determine the Type of Solar Radio Burst (I -V)

Cited by 10 publications

References 1 publication

Moderate Radio Flux Density of Single and Group III Bursts from AR2887 Active Region on 26th October 2021

Moderate Radio Flux Density of Single and Group III Bursts from AR2887 Active Region on 26th October 2021

Development of Large Aperture Microstrip Antenna for Radio Wave Energy Harvesting

Investigation of Characteristics of Noise Storm Solar Burst Type I on 11th March 2013

Contact Info

Product

Resources

About