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Solar radio monitoring · Diamond WD-330S · 10 m Terminated Folded Dipole (T2FD)

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Waiting for RSS data

Live Radio-Sky Spectrograph waterfall from the RSPdx-R2, antenna C. Original RSS colours, normalization and axes. Live reception does not confirm file recording or a solar burst detection.

Display min Display max

Display range is set once from live data; edit it without changing the receiver gain.

Antenna and observation details / Anten bilgileri

Receiving antenna: Diamond WD-330S, 10 m horizontal terminated folded dipole (T2FD), east–west orientation (90°–270°), upper wire 4.00 m and lower wire 3.70 m above wet soil (30 cm separation). Passive Solar and Jovian radio observations at 20.1 MHz.

Antenna pattern: Approximate dipole-like reception model with E–W wire axis (broadside N–S). The actual TFD response depends on installation height, termination and surroundings. The displayed pattern is not a measured gain map.

RSS bridge: 1 s rolling mean, no frequency smoothing, target 5 sweeps/s. This panel shows the original RSS waterfall image, refreshed every 2 seconds; it does not reconstruct or recolour the spectra. Frequency and time axes come from RSS.

ARAS · RADIO MONITORING

Radio-SkyPipe · live chart

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Band average received from RSS. Vertical values are uncalibrated numerical levels.

The SkyPipe chart capture area may not have been selected yet.

The image timestamp alone does not confirm that samples are advancing or being recorded.

NOAA SWPC

Solar Observation Panel

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Sunspot reports, X-ray flux and event times from NOAA. These reference observations are separate from ARAS radio detections.

Solar flare probability · NOAA forecast

Waiting for forecast

Forecast day (UTC)	M-class	X-class
Waiting for forecast

Whole-Sun daily flare probabilities from NOAA SWPC. These are forecasts, not detected events or the probability of receiving a radio burst at ARAS.

GOES X-ray flux · last 6 hours

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0.1–0.8 nm · W/m² · logarithmic scale · UTC

Hover over the chart to read the sample time and flux.

Active regions · NOAA sunspot report

Waiting for report

NOAA AR	Location	Sunspot count	Area (µHem)	Magnetic class
Waiting for data

X-ray flares · NOAA event reports

Source records from the last 24 hours · all times UTC

Class	Start UTC	Peak UTC	End UTC	Region
Waiting for data

Radio burst reports · NOAA/RSTN

Waiting for official report timestamp

RSP: swept-frequency radio events · RBR: fixed-frequency radio events. Station codes and times follow the official report.

Waiting for data

Sources refresh approximately every 5 minutes.

Sources

ARAS · SKY GEOMETRY

WD-330S · Güneş ve Jüpiter

3D · sürükleyerek döndür

İstasyon: 40.988° K, 29.028° D · denizden yaklaşık 50 m. Sabit istasyon koordinatları; ziyaretçinin GPS konumu kullanılmaz.

Tarih (İstanbul)Saat (İstanbul)

Gün içinde gez

Bakış açısı Bakış yüksekliği

Gökcismi	Azimut	Yükseklik	Durum

Yön alanı — ölçülmüş anten lobu değildir

Tel ölçüleri gerçek; turkuaz koni yalnızca ayarlanabilir geometrik planlama alanıdır. Kazanç, −3 dB sınırı veya tespit garantisi vermez. Varsayılan güney / 45° yükseklik / 45° yarı açı, anten hesabından elde edilmemiş bir başlangıç seçimidir.

WD-330S yaklaşık alım loblarını göster

Anten geometrisi ve hesap yöntemi

7,10 m beslenen dipol ve kuzeyinde 2,8 m uzakta 7,45 m reflektör; teller doğu–batı, yerden 4 m. İleri yön güney. Altındaki 4 × 5 m kafes zemine serili, antene elektriksel bağlı değil. Kafesin yönü ve merkezi belirtilmediğinden çizimde temsili yerleştirildi.

Güneş/Jüpiter: Astronomy Engine, istasyona göre topocentric azimut/yükseklik; geometrik ufuk, atmosferik kırılma kapalı. Gökcisimleri ve yolları yön küresinde gösterilir, uzaklık ölçekli değildir. Tel yalıtımı, toprak, kafes, çevre engelleri ve iyonosfer burada modellenmez. Jüpiter'in ufuk üstünde olması radyo patlaması beklendiği anlamına gelmez. Saatler İstanbul (UTC+3); bilgisayar saati doğru olmalıdır.

Astronomy Engine · kaynak ve MIT lisansı

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