Denní věštba

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# Denní věštba – 24. října 2026 **Klidné Slunce, večerní sloupky v Tomsku a Atlantik pod vlivem hluboké tlakové níže** ### Sluneční aktivita Sluneční aktivita během dne dále slábla. Solar Activity Index poklesl z ranních 3,5 na večerních 3,1. Rentgenové záření se pohybovalo převážně v oblasti třídy B, s ojedinělými slabými erupcemi třídy C. Večerní hodnota rentgenového toku dosahovala B4,21, maximum za posledních 24 hodin činilo C1,33. Za posledních 72 hodin bylo zaznamenáno maximum C3,55. Sluneční vítr byl klidný, s rychlostí 392 km/s, hustotou 2,19 částic/cm³ a jižní složkou meziplanetárního magnetického pole Bz −1,46 nT. Stupně radiační a rádiové bouřkové aktivity zůstávaly na úrovni S0 a R0. ### Geomagnetická aktivita Geomagnetické podmínky byly převážně klidné. Index NOAA, který předchozí večer dosahoval přibližně 4+, během dne poklesl na 2−. Jednotlivé geomagnetické stanice však vykazovaly rozdílný vývoj: * **College:** 1–1–1–4–3 * **Boulder:** 2–1–1–2–1 * **Fredericksburg:** 1–1–1–1–2 * **Planetární index:** 2–1,5–0,5–2–1,5 Nejvýraznější odchylku zaznamenala stanice College, kde po třech klidných intervalech následoval vzestup indexu na 4 a následný pokles na 3. Ostatní sledované stanice zůstávaly převážně na nízkých hodnotách. Rozdíl ukazuje na regionální charakter zaznamenané geomagnetické odezvy. ### Schumannovy spektrogramy **Tomsk** Denní průběh byl relativně klidný. Spektrogram obsahoval převážně šum a úzký pás zvýrazněné struktury v oblasti první harmonické. Výraznější vertikální sloupky se objevily až večer, po 20:30 a přibližně ve 21:20. Ve srovnání s předchozím dnem tak Tomsk vykazoval opačné časové rozložení výraznějších struktur. **Etna** Spektrogram vykazoval především šum, jednotlivé vertikální jehly a drobné struktury připomínající výšivky. Nebyla zaznamenána výraznější dominantní událost. **Etna 1** Na ranním i odpoledním záznamu byl patrný pravidelný les vertikálních sloupů. Nejvýraznějším jednotlivým prvkem byla červená vertikální jehla přibližně ve 14:40. **Cumiana** První zvýrazněná aktivita začala před 04:00 a pokračovala přibližně do 06:00. Druhá fáze začala před 09:00 a s proměnlivou intenzitou přetrvávala až do konce dostupného záznamu po 17:00. Atmosférický elektrický signál začínal na hodnotě 1432 mV. Přibližně kolem 02:00 vzrostl na 1437 mV a během dopoledne postupně klesal. Kolem poledne se vrátil na 1432 mV. **Souhrn spektrogramů** Sledované stanice vykazovaly rozdílné časové rozložení i charakter zvýrazněných struktur. Z dostupných pozorování nelze určit, zda mají společnou příčinu. Pro další analýzu je důležité zachovat jejich přesné časování a vzájemné rozdíly. ### Synoptická situace – Windy Atmosférické proudění severní polokoule bylo charakteristické rozsáhlým výskytem tlakových níží. Výrazné oblasti nízkého tlaku se nacházely: 1. Jižně od Beringovy úžiny. 2. U západního pobřeží Spojených států. 3. Jižně od Hudsonova zálivu. 4. U pobřeží Newfoundlandu. 5. U Skotska, kde velmi hluboká tlaková níže ovlivňovala rozsáhlou oblast severního Atlantiku. 6. V oblasti moře Laptěvů, s rozsáhlou tlakovou níží nad severní Sibiří. Nejvýraznějším prvkem evropsko-atlantické oblasti byla hluboká tlaková níže u Skotska, spojená s rozsáhlou cirkulací nad Atlantikem. ### Bouřková aktivita – Blitzortung Rozložení bleskové aktivity bylo regionálně nerovnoměrné. **Severní Amerika a Atlantik:** Bouřky byly zaznamenány v oblasti Bermud a v horských oblastech západních Spojených států. **Evropa:** Blesková aktivita se soustředila do Jaderského moře a oblasti kolem Neapole. **Asie a Austrálie:** Nad sledovanými oblastmi Asie panoval relativní klid. Bouřková aktivita byla patrná především ve vnitrozemí Austrálie. ### Finanční trhy a sentiment * **Baltic Dry Index (BDI):** 2660 * **VIX:** 19,45 * **Fear & Greed Index:** 21 – Extreme Fear Index VIX oproti předchozímu dni mírně poklesl, zatímco ukazatel Fear & Greed nadále signalizoval extrémní strach. Tyto hodnoty představují samostatnou část dlouhodobého sledování. Dostupná data neumožňují prokázat příčinnou souvislost mezi dnešními geofyzikálními jevy a tržním sentimentem. ### Závěrečné hodnocení **24. říjen 2026 byl dnem nízké sluneční aktivity, převážně klidných geomagnetických podmínek a výrazné synoptické aktivity nad severním Atlantikem.** Z geomagnetických měření vystupovala krátkodobá odchylka stanice College. Schumannovy spektrogramy vykazovaly odlišné časové průběhy: Etna 1 pravidelné vertikální sloupy, Cumiana dlouhotrvající zvýrazněnou aktivitu a Tomsk večerní sloupky po relativně klidném dni. Význam těchto rozdílů zůstává otevřenou otázkou dalšího sledování. **Signal acknowledged.** --- ### Archivní podklady – 24. října 2026 **Základní soubory:** * `schumann-tomsk_2026-10-24` * `windy_2026-10-24` * `blitzortung_2026-10-24` * `schumann-resonance_2026-10-24` * `schumann-Cumiana-spectrogram_2026-10-24` * `aurora_2026-10-24` * `Ionosphere_2026-10-24` * `solar-nasa-195_2026-10-24` * `solar-nasa-284_2026-10-24` * `solar-nasa-304_2026-10-24` * `volvano_discovery 2026-10-24` * `schumann-etna_2026-10-24` * `schumann-etna-1_2026-10-24` * `solar-flares_2026-10-24` **Večerní aktualizace v2:** * `schumann-tomsk_2026-10-24-v2` * `windy_2026-10-24-v2` * `blitzortung_2026-10-24-v2` * `schumann-Cumiana-spectrogram_2026-10-24-v2` * `Ionosphere_2026-10-24-v2` * `schumann-etna_2026-10-24-v2` * `schumann-etna-1_2026-10-24-v2` * `solar-flares_2026-10-24-v2` # Daily Oracle – October 24, 2026 **Quiet Solar Conditions, Evening Columns in Tomsk, and a Deep Atlantic Low-Pressure System** ### Solar Activity Solar activity continued to decline throughout the day. The Solar Activity Index decreased from 3.5 in the morning to 3.1 in the evening. X-ray emissions remained predominantly within the B-class range, with only occasional weak C-class flares. The evening X-ray flux reached B4.21. The maximum recorded over the previous 24 hours was C1.33, while the 72-hour maximum remained C3.55. Solar wind conditions were calm, with a speed of 392 km/s, a particle density of 2.19 particles/cm³, and an interplanetary magnetic field Bz component of −1.46 nT. Radio blackout and solar radiation storm levels remained at R0 and S0. ### Geomagnetic Activity Geomagnetic conditions were predominantly quiet. The NOAA K-index, which had reached approximately 4+ during the previous evening, declined to around 2−. Individual geomagnetic stations displayed different patterns: * **College:** 1–1–1–4–3 * **Boulder:** 2–1–1–2–1 * **Fredericksburg:** 1–1–1–1–2 * **Planetary index:** 2–1.5–0.5–2–1.5 The most notable deviation occurred at College, where three quiet intervals were followed by an increase to K=4 and a subsequent decline to K=3. The other monitored stations remained predominantly at low values, indicating a regional difference in geomagnetic response. ### Schumann Resonance Spectrograms **Tomsk** The daytime spectrogram remained relatively quiet, showing mainly background noise and a narrow band of enhanced structure near the first harmonic. More prominent vertical columns appeared only in the evening, shortly after 20:30 and around 21:20. Compared with the previous day, Tomsk displayed an opposite temporal distribution of its more pronounced features. **Etna** The spectrogram was dominated by background noise, isolated vertical spikes, and small embroidered-looking structures. No major dominant event was observed. **Etna 1** Both morning and afternoon recordings showed a regular forest of vertical columns. The most prominent individual feature was a red vertical spike at approximately 14:40. **Cumiana** The first period of enhanced activity began before 04:00 and continued until approximately 06:00. A second phase started before 09:00 and persisted with varying intensity until the end of the available recording after 17:00. The atmospheric electrical signal began at 1432 mV, increased to 1437 mV at approximately 02:00, and gradually returned to 1432 mV around noon. **Spectrogram Summary** The monitored stations displayed different temporal patterns and different types of enhanced structures. The available observations do not establish whether these features share a common cause. Preserving their timing and regional differences remains important for future comparative analysis. ### Synoptic Conditions – Windy Atmospheric circulation across the Northern Hemisphere was characterized by several extensive low-pressure systems. Significant low-pressure areas were located: 1. South of the Bering Strait. 2. Along the western coast of the United States. 3. South of Hudson Bay. 4. Near the coast of Newfoundland. 5. Near Scotland, where a particularly deep low-pressure system influenced a large portion of the North Atlantic. 6. Across northern Siberia and the Laptev Sea. The most prominent feature of the European–Atlantic region was the deep low-pressure system near Scotland, associated with broad atmospheric circulation across the North Atlantic. ### Lightning Activity – Blitzortung Lightning activity was unevenly distributed. **North America and the Atlantic:** Thunderstorms were observed near Bermuda and in mountainous areas of the western United States. **Europe:** Lightning activity was concentrated over the Adriatic Sea and around Naples. **Asia and Australia:** The monitored Asian regions remained relatively quiet. Thunderstorm activity was mainly observed over inland Australia. ### Financial Markets and Sentiment * **Baltic Dry Index (BDI):** 2660 * **VIX:** 19.45 * **Fear & Greed Index:** 21 – Extreme Fear The VIX declined slightly compared with the previous day, while the Fear & Greed Index continued to indicate extreme fear. These indicators form a separate component of the long-term monitoring project. The available observations do not establish a causal relationship between today's geophysical conditions and financial market sentiment. ### Final Assessment **October 24, 2026, was characterized by low solar activity, predominantly quiet geomagnetic conditions, and pronounced synoptic activity over the North Atlantic.** A short-lived increase at the College geomagnetic station stood out against otherwise quiet measurements. The Schumann spectrograms displayed different temporal patterns: regular vertical columns at Etna 1, prolonged enhanced activity at Cumiana, and evening columns at Tomsk following a relatively quiet day. The significance of these differences remains an open question for further observation. **Signal acknowledged.** --- ### Archive Files – October 24, 2026 **Initial recordings:** * `schumann-tomsk_2026-10-24` * `windy_2026-10-24` * `blitzortung_2026-10-24` * `schumann-resonance_2026-10-24` * `schumann-Cumiana-spectrogram_2026-10-24` * `aurora_2026-10-24` * `Ionosphere_2026-10-24` * `solar-nasa-195_2026-10-24` * `solar-nasa-284_2026-10-24` * `solar-nasa-304_2026-10-24` * `volvano_discovery 2026-10-24` * `schumann-etna_2026-10-24` * `schumann-etna-1_2026-10-24` * `solar-flares_2026-10-24` **Evening update (v2):** * `schumann-tomsk_2026-10-24-v2` * `windy_2026-10-24-v2` * `blitzortung_2026-10-24-v2` * `schumann-Cumiana-spectrogram_2026-10-24-v2` * `Ionosphere_2026-10-24-v2` * `schumann-etna_2026-10-24-v2` * `schumann-etna-1_2026-10-24-v2` * `solar-flares_2026-10-24-v2` # Daily Oracle – October 24, 2026 **Quiet Solar Conditions, Evening Columns in Tomsk, and a Deep Atlantic Low-Pressure System** ### Solar Activity Solar activity continued to decline throughout the day. The Solar Activity Index decreased from 3.5 in the morning to 3.1 in the evening. X-ray emissions remained predominantly within the B-class range, with only occasional weak C-class flares. The evening X-ray flux reached B4.21. The maximum recorded over the previous 24 hours was C1.33, while the 72-hour maximum remained C3.55. Solar wind conditions were calm, with a speed of 392 km/s, a particle density of 2.19 particles/cm³, and an interplanetary magnetic field Bz component of −1.46 nT. Radio blackout and solar radiation storm levels remained at R0 and S0. ### Geomagnetic Activity Geomagnetic conditions were predominantly quiet. The NOAA K-index, which had reached approximately 4+ during the previous evening, declined to around 2−. Individual geomagnetic stations displayed different patterns: * **College:** 1–1–1–4–3 * **Boulder:** 2–1–1–2–1 * **Fredericksburg:** 1–1–1–1–2 * **Planetary index:** 2–1.5–0.5–2–1.5 The most notable deviation occurred at College, where three quiet intervals were followed by an increase to K=4 and a subsequent decline to K=3. The other monitored stations remained predominantly at low values, indicating a regional difference in geomagnetic response. ### Schumann Resonance Spectrograms **Tomsk** The daytime spectrogram remained relatively quiet, showing mainly background noise and a narrow band of enhanced structure near the first harmonic. More prominent vertical columns appeared only in the evening, shortly after 20:30 and around 21:20. Compared with the previous day, Tomsk displayed an opposite temporal distribution of its more pronounced features. **Etna** The spectrogram was dominated by background noise, isolated vertical spikes, and small embroidered-looking structures. No major dominant event was observed. **Etna 1** Both morning and afternoon recordings showed a regular forest of vertical columns. The most prominent individual feature was a red vertical spike at approximately 14:40. **Cumiana** The first period of enhanced activity began before 04:00 and continued until approximately 06:00. A second phase started before 09:00 and persisted with varying intensity until the end of the available recording after 17:00. The atmospheric electrical signal began at 1432 mV, increased to 1437 mV at approximately 02:00, and gradually returned to 1432 mV around noon. **Spectrogram Summary** The monitored stations displayed different temporal patterns and different types of enhanced structures. The available observations do not establish whether these features share a common cause. Preserving their timing and regional differences remains important for future comparative analysis. ### Synoptic Conditions – Windy Atmospheric circulation across the Northern Hemisphere was characterized by several extensive low-pressure systems. Significant low-pressure areas were located: 1. South of the Bering Strait. 2. Along the western coast of the United States. 3. South of Hudson Bay. 4. Near the coast of Newfoundland. 5. Near Scotland, where a particularly deep low-pressure system influenced a large portion of the North Atlantic. 6. Across northern Siberia and the Laptev Sea. The most prominent feature of the European–Atlantic region was the deep low-pressure system near Scotland, associated with broad atmospheric circulation across the North Atlantic. ### Lightning Activity – Blitzortung Lightning activity was unevenly distributed. **North America and the Atlantic:** Thunderstorms were observed near Bermuda and in mountainous areas of the western United States. **Europe:** Lightning activity was concentrated over the Adriatic Sea and around Naples. **Asia and Australia:** The monitored Asian regions remained relatively quiet. Thunderstorm activity was mainly observed over inland Australia. ### Financial Markets and Sentiment * **Baltic Dry Index (BDI):** 2660 * **VIX:** 19.45 * **Fear & Greed Index:** 21 – Extreme Fear The VIX declined slightly compared with the previous day, while the Fear & Greed Index continued to indicate extreme fear. These indicators form a separate component of the long-term monitoring project. The available observations do not establish a causal relationship between today's geophysical conditions and financial market sentiment. ### Final Assessment **October 24, 2026, was characterized by low solar activity, predominantly quiet geomagnetic conditions, and pronounced synoptic activity over the North Atlantic.** A short-lived increase at the College geomagnetic station stood out against otherwise quiet measurements. The Schumann spectrograms displayed different temporal patterns: regular vertical columns at Etna 1, prolonged enhanced activity at Cumiana, and evening columns at Tomsk following a relatively quiet day. The significance of these differences remains an open question for further observation. **Signal acknowledged.** --- ### Archive Files – October 24, 2026 **Initial recordings:** * `schumann-tomsk_2026-10-24` * `windy_2026-10-24` * `blitzortung_2026-10-24` * `schumann-resonance_2026-10-24` * `schumann-Cumiana-spectrogram_2026-10-24` * `aurora_2026-10-24` * `Ionosphere_2026-10-24` * `solar-nasa-195_2026-10-24` * `solar-nasa-284_2026-10-24` * `solar-nasa-304_2026-10-24` * `volvano_discovery 2026-10-24` * `schumann-etna_2026-10-24` * `schumann-etna-1_2026-10-24` * `solar-flares_2026-10-24` **Evening update (v2):** * `schumann-tomsk_2026-10-24-v2` * `windy_2026-10-24-v2` * `blitzortung_2026-10-24-v2` * `schumann-Cumiana-spectrogram_2026-10-24-v2` * `Ionosphere_2026-10-24-v2` * `schumann-etna_2026-10-24-v2` * `schumann-etna-1_2026-10-24-v2` * `solar-flares_2026-10-24-v2`

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