НОВИНИ
Репітер проходжень DX
Сторінка транслює інформацію, яку ретельно підібрав Paul L Herrman aka N0NBH. Дані для умов УКХ-зв’язку отримані від DXrobot Gouda, Make More Miles on VHF та Andy aka G7IZU.
Файли з поміткою new розміщені, або змінені менше місяця тому. Вся інформація, крім службової, доступна для завантаження. Кількість переглядів сторінки - 55
Поточні умови проходжень
В Україні 12 жовтня, 2025 року. Дані, що надійшли протягом останніх 5 хвилин показані нижче. Репітер постійно збирає інформацію з різних сайтів, тому сторінка буде автоматично оновлена через 5:00 хвилин за умови, що вона активна.
| Item | Day | Night | |
|---|---|---|---|
| Band 80m-40m | Poor | Fair | |
| Band 30m-20m | Good | Good | |
| Band 17m-15m | Good | Good | |
| Band 12m-10m | Fair | Poor |
| Item | Data | Item | Data |
|---|---|---|---|
| Es America N | Band Closed | Aurora Lat | 65.6° |
| Es Europe 2m | Band Closed | Aurora active | 3/n=1.99 |
| Es Europe 4m | Band Closed | Aurora North | Band Closed |
| Es Europe 6m | Band Closed | ||
| Item | Data | Item | Data |
|---|---|---|---|
| Solar flux | 131 | Sunspots | 101 |
| A-index | 17 | K-index | 3 |
| X-Ray | C9.2 | 304A | 133.0 |
| P-flux | 219 | E-flux | 1520 |
| Mag field (Bz) | 2.4 | Solar wind | 679.9 |
| Geomag field | UNSETTLD | Sig noise | S2-S3 |
| MUF US | NoRpt | foF2 US | Array |
Дані з сайту N0NBH hamqsl.com від 2025-10-12 14:15:29 за часом GMT. Прямі посилання на файли з нашого ресурсу доступні у кількох форматах: XML [1.6 Kb], RSS [2 Kb], JSON [617 b]
Файли кешуються на сервері та оновлюються щогодини, крім того, на додаток до RSS та XML, ми генеруємо файл у форматі JSON для вільного користовування за умови посилань на джерела.
Дешифрування таблиці прогнозу проходжень
| Category | Radio Blackouts Use X-Ray | Solar Radiation Storms Use Proton Flux | Geomagnetic Storms Use K-Index/K-nT/ Aurora/Solar Wind/Bz | Band Openings Use Solar Flux (SN) | Electron Alert Use Electron Flux | |
| Extreme | X20(1 per cycle) Complete HF blackout on entire sunlit side lasting hours | 1000000 (1 per cycle) Complete HF blackout in polar regions | K=9 (nT=>500) [Aur=10++] (SW=>800) [Bz=-40 -50] (4 per cycle) HF impossible. Aurora to 40°. Noise S30+. | 200-300 (SN=160-250) Reliable communications all bands up through 6m | >1000 Alert Partial to complete HF blackout in polar regions | |
| Severe | X10 (8 per cycle) HF blackout on most of sunlit side for 1 to 2 hours | 100000 (3 per cycle) Partial HF blackout in polar regions | K=8 (nT=330-500) [Aur=10+] (SW=700-800) [Bz=-30 -40] (100 per cycle) HF sporadic. Aurora to 45°. Noise S20-S30. | |||
| Strong | X1 (175 per cycle) Wide area HF blackout for about an hour on sunlit side | 10000 (10 per cycle) Degraded HF propagation in polar regions | K=7 (nT=200-330) [Aur=10] (SW=600-700) [Bz=-20 -30] (200 per cycle) HF intermittent. Aurora to 50°. Noise S9-S20. | 150-200 (SN=105-160) Excellent conditions all bands up through 10m w/6m openings | ||
| Moderate | M5 (350 per cycle) Limited HF blackout on sunlit side for tens of minutes | 1000 (25 per cycle) Small effects on HF in polar regions | K=6 (nT=120-200) [Aur=9] (SW=500-600) [Bz=-10 -20] (600 per cycle) HF fade higher lats. Aurora to 55°. Noise S6-S9. | 120-150 (SN=70-105) Fair to good conditions all bands up through 10m | <1000 Active Degraded HF propagation in polar regions | |
| Minor | M1 (2000 per cycle) Occasional loss of radio contact on sunlit side | 100 (50 per cycle) Minor impacts on HF in polar regions | K=5 (nT=70-120) [Aur=8] (SW=400-500) [Bz=0 -10] (1700 per cycle) HF fade higher lats. Aurora to 56°. Noise S4-S6. | 90-120 (SN=35-70) Fair conditions all bands up through 15m | <100 Active Minor impacts on HF in polar regions | |
| Active | C1 Moderate Flare Low absorption of HF signals | 10 Active Very minor impacts on HF in polar regions | K=3-4 (nT=20-70) [Aur=6-7] (SW=200-400) [Bz=0-+50] Unsettled/Active Minor HF fade higher lats. Aurora 60-58°. Noise S2-S3. | 70-90 (SN=10-35) Poor to fair conditions all bands up through 20m | <10 Normal No impacts on HF | |
| Normal | A1-B9 No/Small Flare No or very minor impact to HF signals | 1 Normal No impacts on HF | K=0-2 (nT=0-20) [Aur=<5] (SW=200-400) [Bz=0-+50] Inactive/Quiet No impacts on HF. Aurora 67-62°. Noise S0-S2. | 64-70 (SN=0-10) Bands above 40m unusable | <1 Normal No impacts on HF | |
VHF Conditions Aurora Lat (Auroral Latitude): Indicates lowest latitude from the current Aurora Activity measurement. Text color coded for low activity, hi-latitude, & mid-latitude.Aurora (Northern Auroral Activity): Band Closed = No/Low Auroral activity. High LAT AUR = Auroral activity >60°N. MID LAT AUR = Auroral activity 60° to 30°N. EsEU (Sporadic E - Europe): Band Closed = No Sporadic E (ES) activity. High MUF (2M only) = Cond support 2M ES 50/70/144MHz ES = Respective band open EsNA (Sporadic E - North America): Band Closed = No Sporadic E (ES) activity. High MUF = Cond support 2M ES 144MHz ES = ES reported @ 2M EME (Earth-Moon-Earth): Current EME degradation. Very Poor (>5.5dB), Poor (4dB), Moderate (2.5dB), Good (1.5dB), Very Good (1dB), Excellent (<1dB). Solar Flare Probability: Provides the probability of a solar flare (in %) for the net 24 hours. MUF (Max Usable Frequency Bar Color): No Sporadic E (ES) activity / ES reported @ 6M / ES reported @ 4M / Cond support 2M ES / ES reported @ 2M MS (Meteor Scatter) Activity Color bar: Provides meteor activity color coded MIN to MAX conditions (see the graph below the bar). | ||||||
Глосарій термінів прогнозу проходжень
| Item | Element | Description | |||
|---|---|---|---|---|---|
| SFI | Solar Flux Index | DRAO Penticton no longer available, using NOAA data. Intensity of solar radiation measured at 2800MHz (10.7cm). Good indication of the F layer ionization (layer that gives us most of our DX on HF). The higher the number, the greater the level of ionization is, and the higher the frequency. Measured once daily. Note that NOAA recorded SFI for the day is the 2nd (or middle) of the DRAO readings. SFI does correlate to 304A (see graph below). | |||
| SN | Sunspot Number | Sunspot Number provided by NOAA is a reported value from 0 to 250. It is computed using a formula [R=k (10g+s)] by Rudolph Wolf in 1848, where R is the sunspot number; g is the number of sunspot groups on the solar disk; s is the total number of individual spots in all the groups; and k is a variable scaling factor (usually less than 1) that accounts for observing conditions and the type of observing device. NOAA SN does loosely correlate to SFI. Updated once daily. | |||
| SNeX | NWRA Effective Smoothed Sunspot Number | Three measurements are available for this parameter calculated by NorthWest Research Associates, Inc. The NWRA values (used with permission) are available for Global (SNeG), Northern Hemisphere (SNeN) and Southern Hemisphere (SNeS) and are calculated using foF2 data from NOAA/NCEI. In addition, the color of the label (SNeX) determines the validity of the data (last f0f2 observations from NOAA). Green SNeX = no more than 1 hour ago. Yellow SNeX = no more than 4 hours ago. Orange SNeX = no more than 12 hours ago. Red SNeX = more than 12 hours ago. They are updated once every hour. See NWRA site for a in depth background on the SSNe parameter. | |||
| A | Planetary A Index | NOAA reported value from 0 to 400. Provides a daily average level for geomagnetic activity. Uses the average of eight 3 hour K-Index values (magnetic value measured in nanotesla or nT) to provide the level of instability in the earth’s geomagnetic field. When used with K-Index: Both high indicates geomagnetic field is unstable, and HF signals are prone to sudden fades, and some paths may close while others open up abruptly and with little warning. High K index/Low A indicates a sudden, abrupt disturbance in the geomagnetic field, which can cause an intense but brief disruption in HF propagation, but can cause an auroral event. Updated once daily. | |||
| K | Planetary K Index | NOAA reported value from 0 to 9. Measures disturbances in the horizontal component of earth`s magnetic field. Value in nT is measured using a magnetometer during a three-hour interval, and then converted to a factor. Use with A-Index – sees above to determine HF conditions. Updated eight times daily. | |||
| X-Ray or XRY | Hard X-Rays | NOAA reported value from A0.0 to X9.9. Intensity of hard x-rays hitting the earth’s ionosphere. Impacts primarily the D-layer (HF absorption). The letter indicates the order of magnitude of the X-rays (A, B, C, M and X), where A is the lowest. The number further defines the level of radiation. Updated eight times daily. | |||
| 304A | 304 Angstroms | NOAA reported value from 0 to unknown. Relative strength of total solar radiation at a wavelength of 304 angstroms (or 30.4 nm), emitted primarily by ionized helium in the sun`s photosphere. Two measurements are available for this parameter, one measured by the Solar Dynamics Observatory, using the EVE instrument, and the other, using data from the SOHO satellite, using its SEM instrument. Responsible for about half of all the ionization of the F layer in the ionosphere. 304A does correlate to SFI (see graph below). Updated hourly. | |||
| Pnt Flx or PF | Proton Flux | NOAA reported value from 0 to unknown. Density of charged protons in the solar wind. The higher the numbers, the more the impact the ionosphere. Primarily impacts the E-Layer of the ionosphere. Updated hourly. | |||
| Elc Flx or EF | Electron Flux | NOAA reported value from 0 to unknown. Density of charged electrons in the solar wind. The higher the numbers (>1000), the more the impact the ionosphere. Primarily impacts the E-Layer of the ionosphere. Updated hourly. | |||
| Aur | Aurora | Data is now calculated from the current hemispheric power value (0-150 GW) to give the old reported scaled factor value from 0 to 10++. Indicates how strong the F-Layer ionization is in the polar regions. Higher values cause auroral events (including northern/southern lights) to move to lower latitude. Updated every 15 minutes. | |||
| n | Normalization | Always 1.99 now that Aur is calculated. Will be removed on the next major banner update. | |||
| Bz | Bz Component | ACE Satellite reported value from +50 to -50. Strength and direction of the interplanetary magnetic field as impacted by solar activity. Positive is same direction as the earth`s magnetic field, and negative is the opposite magnetic polarity. Cancels out earth’s magnetic field when negative, which increases the impact of solar particles in the ionosphere. Updated hourly. | |||
| SW | Solar Wind | ACE Satellite reported value from 0 to 1000. Speed (kilometers per second) of the charged particles as they pass earth. The higher the speed, the greater the pressure is exerted on the ionosphere. Values greater than 500 km/sec have impact on HF communications. Updated hourly. | |||
| Aur Lat | Aurora Latitude | Calculated value from 67.5 to <45.0. Calculation from NOAA utilizes the current Aurora measurement. Used to estimate the lowest latitude impacted by the auroral event. Updated every 15 minutes. | |||
| Aur | Aurora | DX-Robot reported event (used with permission). Reports Band Closed for No/Low Auroral activity, High LAT AUR for Auroral activity >60°N, or MID LAT AUR for Auroral activity from 60° to 30°N. Updated every ½ hour. | |||
| EsEU | Sporadic E Europe | DX-Robot reported event (used with permission). Reports Band Closed, High MUF when 2M only is open, or 50/70/144MHz ES when the respective band is reported open. Updated every ½ hour. | |||
| EsNA | Sporadic E North America | DX-Robot reported event (used with permission). Reports Band Closed, High MUF when conditions support Es, and 144MHz ES when the band is reported open. Updated every ½ hour. | |||
| EME Deg | Earth-Moon-Earth Degradation | Make More Miles reported value (used with permission). Reports EME path attenuation as Very Poor (>5.5dB), Poor (4dB), Moderate (2.5dB), Good (1.5dB), Very Good (1dB), Excellent (<1dB). Updated every ½ hour. | |||
| Solar Flare Prob | Solar Flare Probability | University of Bradford predicted value (used with permission). Reports the probability (in %) of a solar flare within the next 24 hours (0-100%). Updated every hour. | |||
| MUF | Maximum Usable Frequency | Make More Miles reported value (used with permission). Provides the Maximum Usable Frequency in a colored bar. Gray indicates No Sporadic E (ES) activity, blue indicates ES reported @ 6M, green indicates ES reported @ 4M, yellow indicates conditions support 2M ES, and red indicates reported @ 2M. Updated every ½ hour. | |||
| MS | Meteor Scatter Activity Bar | Make More Miles reported value (used with permission). Provides the Meteor Scatter activity in a colored bar. Gray indicates no activity. See the color coded graph at the bottom of the bar for activity level. Updated every 1/4 hour. | |||
| GeoMag Fld | Geomagnetic Field | Calculated value. Indicates how quiet or active the earth`s magnetic field is based on the K-Index value. Reports as Inactive, Very Quite, Quiet, Unsettled, Active, Minor Storm, Major Storm, Severe Storm, or Extreme Storm. Higher indications can cause HF blackouts and auroral events. Updated every three hours. | |||
| Sig Noise Lvl | Signal Noise Level | Calculated value. Indicates how much noise (in S-units) is being generated by interaction between the solar wind and the geomagnetic activity. A more active and disturbed solar wind, the greater the noise. Updated every ½ hour. | |||
| MUF | Maximum Usable Frequency | NOAA reported value from 0 to 100MHz. Provides the maximum usable frequency in MHz at one of 11 locations worldwide. Updated every 15 minutes. | |||
| CME | Coronal Mass Ejection | NOAA/SWPC predicted date and time (in UTC). Provides the date and time of a predicted earth bound CME event. Color coded for severity, where green is minor, yellow is moderate, and red is severe. Updated when predictions are received from NOAA/SWPC. | |||
Iоносферні MUF/foF2 у реальному часі
Карта поширення MUF – найвищої частоти, яка буде відбиватися від іоносфери на шляху довжиною 3000 км. Таким чином, MUF уздовж шляху між двома точками показує можливість довгого стрибка DX між ними в даному діапазоні. Якщо MUF становить 12 МГц, то 30 метрів і довше буде працювати, але 20 метрів і коротше не буде. Для довгих маршрутів з кількома стрибками найгірший MUF будь-де на шляху має значення. Для маршрутів з одним стрибком коротше 3000 км корисна частота буде меншою, ніж MUF, тому що сигнали з більшим кутом легше «пробивають» іоносферу. Коли ви наближаєтеся до вертикалі, корисна частота падає до критичної частоти (foF2).
Карта поширення foF2 подібна до карти MUF, за винятком того, що вона відображає критичну частоту (foF2). Тобто найвищу частоту, яку ви можете використовувати для NVIS (зв’язок Skywave «у своєму дворі»). Коли foF2 сягає 7 МГц і вище, то 40 метрів "коротшають" і можуть бути доступні для місцевих контактів; якщо вона опускається нижче 3 МГц, то 80 метрів "довшають" і місцеві станції зникають, хоча віддалені все ще можуть бути досяжними.
Активність VHF/HF у реальному часі
Карта поширення КХ (HF) у реальному часі показує радіостанції, що працюють на 11 діапазонах між 1,8 і 54 МГц. Дисплей показує активність у всьому світі за останні 15 хвилин і автоматично оновлюється щохвилини. Для перегляду графіки у реальному часі потрібно ввімкнути Javascript.
Карта поширення УКХ (VHF) у реальному часі показує радіостанції, що працюють в діапазоні 144 МГц. Вона використовує дані, зібрані системою автоматичного пакетного звітування Інтернет-службою (APRS-IS) із станцій пакетної передачі в аматорській радіослужбі. Карта показує активність за останню годину. Для перегляду графіки у реальному часі потрібно ввімкнути Javascript
Примітки
Аматорські радіопередачі визначено як суспільне надбання. Будь-хто може отримати їх, а також повторно передавати, публікувати чи зберігати, як вважає за потрібне. Якщо ви не бажаєте, щоб ваша позиція була кимось опублікована в Інтернеті, єдиний гарантований спосіб – не передавати її.
[En] The repeater shows information carefully selected by Paul L Herrman aka N0NBH. In addition to the RSS and XML formats, we generate a JSON file that can be freely used, provided that the original sources mentioned above are referenced.