From: will Date: Thu, 23 May 2024 18:32:53 +0000 (+0100) Subject: added .mp3 compressed version for lower internet connections X-Git-Url: https://git.ozva.co.uk/?a=commitdiff_plain;p=spaceweather added .mp3 compressed version for lower internet connections --- diff --git a/config/last b/config/last index 273bdc5..a5dca55 100644 --- a/config/last +++ b/config/last @@ -1,7 +1,7 @@ -Welcome to space weather, issued by XMDV radio at Mon the 20 May 2024 at 12:30:08 -In the last 24 hours Solar activity reached moderate levels when Region 3685 produced an M1.9 to 1N at 19 to 1344 utc, an M2.5 to 1B at 19 to 1756 utc, and an M1.6 to 1 n at 19 to 2159 utc. Growth was observed in theintermediate spots of Region 3685 and the leader spots of Region 3683 . New Region 3687 was numbered. Modelling of a filament eruption coronal mass ejection mentioned in the 19 to 1230 utcdiscussion suggested passage well south of the ecliptic. Analysis andmodelling are underway for a halo coronal mass ejection first seen in C2 imagery at 20 to 0536 utc. This event is associated with a C6.7 flare at 20 to 0554 utcfrom AR 3683. Early estimated speeds indicate a possible arrival on 22May. Solar activity is likely to be moderate, with isolated M-class flares probable and a slight chance for an X-class flare on 20 to 22 may. -In the last 24 hours The 10 mega electron volt proton flux at geosynchronous orbit had returned tobackground levels. Electrons greater than 2 mega electron volt at geosynchronous orbitreached a peak level of 406 pfu. There is a slight chance for the greater than 10 mega electron volt protons reaching S1 levels on 20 to 22 may due to the flare potential of Region 3685. The greater than 2 mega electron volt electron flux is expected to remain at normal tomoderate levels, with a chanced for high levels, through 21 may. -In the last 24 hours Solar wind speeds slowly decreased from ~400 to 350 kilometers per second. Total IMFreached 9 nano tesla at 19 to 1417 utc. The maximum southward component of Bzreached to 8 nano tesla at 19 to 1254Z and was mostly southward from around 19 to 00 utcto 19 to 19 utc. Phi was mostly positive. Solar wind enhancements are then expected on 20 may from the coronal mass ejection thatleft the Sunday on 17 may. coronal mass ejection influences are expected to slowly diminishon 21 may. Enhanced conditions are expected on 22 may due to thepossible arrival of a halo coronal mass ejection from 20 may. -In the last 24 hours The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. On 20 May, unsettled to active levels are expected, with G1 storming likely with glancing coronal mass ejection effects from the 17 may coronal mass ejection. Mid tolate day on 21 May, active levels are expected to decrease to mostlyunsettled levels as coronal mass ejection effects gradually diminish. G1-G3 storm levels are possible on 22 may due to the possiblearrival of the 20 may halo coronal mass ejection. -This has been space weather, issued by XMDV radio at Mon the 20 May 2024 at 12:30:08 +Welcome to space weather, issued by XMDV radio at Thu the 23 May 2024 at 12:30:08 +In the last 24 hours Solar activity was moderate with multiple M-class flares. Background X-ray flux was at C-class levels and six designated sunspotgroups were present on the visible solar disk. The most notabledevelopment was areal growth in Region 3679 and the emergence of a delta. This region produced themajority of the activity during the period including the largest flare, an M4.2 flare at 23 to 0216 utc. Region 3683 rotated beyondthe limb, but still managed a C9.7 flare at 23 to 0642 utc. Region 3685 exhibited decay in its intermediate spots. Anew area of potential spot emergence was noted at approximately N20W44, but we are awaiting duration requirements before designation. The restof the spotted regions were mostly inactive. There were two filament eruptions that lifted off the SE. The first oneis first visible in C2 imagery at 23 to 0125 utc. Modeling results showed amiss south and behind Earths orbit. The second originated from justeast of AR 3685 and is first visible in C2 at 23 to 0648 utc. Modeling isunderway for this event at the time of this writing. Solar activity is likely to remain moderate 23 to 25 May, with a slightchance of X-class flares due primarily to the increasingflare potential of Region 3679. +In the last 24 hours The greater than 2 mega electron volt electron flux was normal to moderate and thegreater than 10 mega electron volt proton flux remained at background values. Normal to moderate levels, with a chance for high levels is forecast for 23 to 25 May, while the greater than 10 mega electron volt proton flux is expected tocontinue at background levels. However, there remains a slight chance ofan S1 solar radiation storm due to the potential from Region 3679. +In the last 24 hours Solar wind parameters were slightly enhanced. Total field was primarily 6 to 8 nano tesla, with a peak of 9 nano tesla and the Bz component was variable. Solarwind speed was below 400 kilometers per second. The phi angle was primarily positive. The mildly enhanced IMF is expected to continue on 23 may. Influencesfrom an isolated coronal hole high speed stream are anticipated on 24 to 25 may. However, most ofthe HSS will likely be north of Earth and mainly modest solar wind speedincreases are expected. +In the last 24 hours The geomagnetic field was quiet. The geomagnetic field is expected to be mainly quiet, with isolatedunsettled conditions on 23 may as the minor enhancement in the solarwind continues. coronal hole high speed stream effects 24 to 25 may may lead to additionalunsettled periods, with possible active conditions on 24 may. +This has been space weather, issued by XMDV radio at Thu the 23 May 2024 at 12:30:08 Space weather was created by William Greenwood with material from the N O double A \ No newline at end of file diff --git a/index.html b/index.html index ff065d0..51e4b9b 100644 --- a/index.html +++ b/index.html @@ -1,6 +1,9 @@ + + + Spaceweather @@ -18,7 +21,7 @@

Spaceweather

Welcome to Spaceweather, a daily report of current heliospheric conditions, issued by XMDV Radio and supported by Ozone-Value Holdings.

- +

Transcript (HTML/plaintext)

Spaceweather is generated daily, at time-of-issue of the NOAA's description of the latest solar activity [1]. This data is processed into the spoken portion of the report. In addition, the ambient backing of the report is generated using NOAA X-Ray data from two different satellite sources. @@ -63,7 +66,7 @@

Boston: "[...] we are working with the auroral current. How do you receive my writing?"
- Portland: "Better than with our batteries on. – Current comes and goes gradually." + Portland: "Better than with our batteries on. - Current comes and goes gradually."

© Ozone-Value Holdings 2024

diff --git a/spaceweather.py b/spaceweather.py index 0053de4..5bcdda9 100755 --- a/spaceweather.py +++ b/spaceweather.py @@ -240,6 +240,7 @@ print("finalizing...") os.system(f"sox --effects-file=config/voice.effects {order[-1]['file']} audio/last.wav") os.system(f"sox --combine mix-power audio/voice.wav audio/bed.wav audio/body.wav") os.system(f"sox --effects-file=config/master.effects audio/start.wav audio/body.wav audio/end.wav audio/last.wav spaceweather.wav") +os.system("sox spaceweather.wav --compression 0.7 spaceweather.mp3") print("generated spaceweather!") diff --git a/template.html b/template.html index c6e8aea..a6d26a8 100644 --- a/template.html +++ b/template.html @@ -21,7 +21,7 @@

Spaceweather

Welcome to Spaceweather, a daily report of current heliospheric conditions, issued by XMDV Radio and supported by Ozone-Value Holdings.

- +

Transcript (HTML/plaintext)

Spaceweather is generated daily, at time-of-issue of the NOAA's description of the latest solar activity [1]. This data is processed into the spoken portion of the report. In addition, the ambient backing of the report is generated using NOAA X-Ray data from two different satellite sources. diff --git a/transcript.html b/transcript.html index 4ced6f2..937f4b2 100644 --- a/transcript.html +++ b/transcript.html @@ -1 +1 @@ -

Welcome to space weather, issued by XMDV radio at Mon the 20 May 2024 at 12:30:08

In the last 24 hours Solar activity reached moderate levels when Region 3685 produced an M1.9 to 1N at 19 to 1344 utc, an M2.5 to 1B at 19 to 1756 utc, and an M1.6 to 1 n at 19 to 2159 utc. Growth was observed in theintermediate spots of Region 3685 and the leader spots of Region 3683 . New Region 3687 was numbered. Modelling of a filament eruption coronal mass ejection mentioned in the 19 to 1230 utcdiscussion suggested passage well south of the ecliptic. Analysis andmodelling are underway for a halo coronal mass ejection first seen in C2 imagery at 20 to 0536 utc. This event is associated with a C6.7 flare at 20 to 0554 utcfrom AR 3683. Early estimated speeds indicate a possible arrival on 22May. Solar activity is likely to be moderate, with isolated M-class flares probable and a slight chance for an X-class flare on 20 to 22 may.

In the last 24 hours The 10 mega electron volt proton flux at geosynchronous orbit had returned tobackground levels. Electrons greater than 2 mega electron volt at geosynchronous orbitreached a peak level of 406 pfu. There is a slight chance for the greater than 10 mega electron volt protons reaching S1 levels on 20 to 22 may due to the flare potential of Region 3685. The greater than 2 mega electron volt electron flux is expected to remain at normal tomoderate levels, with a chanced for high levels, through 21 may.

In the last 24 hours Solar wind speeds slowly decreased from ~400 to 350 kilometers per second. Total IMFreached 9 nano tesla at 19 to 1417 utc. The maximum southward component of Bzreached to 8 nano tesla at 19 to 1254Z and was mostly southward from around 19 to 00 utcto 19 to 19 utc. Phi was mostly positive. Solar wind enhancements are then expected on 20 may from the coronal mass ejection thatleft the Sunday on 17 may. coronal mass ejection influences are expected to slowly diminishon 21 may. Enhanced conditions are expected on 22 may due to thepossible arrival of a halo coronal mass ejection from 20 may.

In the last 24 hours The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. On 20 May, unsettled to active levels are expected, with G1 storming likely with glancing coronal mass ejection effects from the 17 may coronal mass ejection. Mid tolate day on 21 May, active levels are expected to decrease to mostlyunsettled levels as coronal mass ejection effects gradually diminish. G1-G3 storm levels are possible on 22 may due to the possiblearrival of the 20 may halo coronal mass ejection.

This has been space weather, issued by XMDV radio at Mon the 20 May 2024 at 12:30:08

Space weather was created by William Greenwood with material from the N O double A

\ No newline at end of file +

Welcome to space weather, issued by XMDV radio at Thu the 23 May 2024 at 12:30:08

In the last 24 hours Solar activity was moderate with multiple M-class flares. Background X-ray flux was at C-class levels and six designated sunspotgroups were present on the visible solar disk. The most notabledevelopment was areal growth in Region 3679 and the emergence of a delta. This region produced themajority of the activity during the period including the largest flare, an M4.2 flare at 23 to 0216 utc. Region 3683 rotated beyondthe limb, but still managed a C9.7 flare at 23 to 0642 utc. Region 3685 exhibited decay in its intermediate spots. Anew area of potential spot emergence was noted at approximately N20W44, but we are awaiting duration requirements before designation. The restof the spotted regions were mostly inactive. There were two filament eruptions that lifted off the SE. The first oneis first visible in C2 imagery at 23 to 0125 utc. Modeling results showed amiss south and behind Earths orbit. The second originated from justeast of AR 3685 and is first visible in C2 at 23 to 0648 utc. Modeling isunderway for this event at the time of this writing. Solar activity is likely to remain moderate 23 to 25 May, with a slightchance of X-class flares due primarily to the increasingflare potential of Region 3679.

In the last 24 hours The greater than 2 mega electron volt electron flux was normal to moderate and thegreater than 10 mega electron volt proton flux remained at background values. Normal to moderate levels, with a chance for high levels is forecast for 23 to 25 May, while the greater than 10 mega electron volt proton flux is expected tocontinue at background levels. However, there remains a slight chance ofan S1 solar radiation storm due to the potential from Region 3679.

In the last 24 hours Solar wind parameters were slightly enhanced. Total field was primarily 6 to 8 nano tesla, with a peak of 9 nano tesla and the Bz component was variable. Solarwind speed was below 400 kilometers per second. The phi angle was primarily positive. The mildly enhanced IMF is expected to continue on 23 may. Influencesfrom an isolated coronal hole high speed stream are anticipated on 24 to 25 may. However, most ofthe HSS will likely be north of Earth and mainly modest solar wind speedincreases are expected.

In the last 24 hours The geomagnetic field was quiet. The geomagnetic field is expected to be mainly quiet, with isolatedunsettled conditions on 23 may as the minor enhancement in the solarwind continues. coronal hole high speed stream effects 24 to 25 may may lead to additionalunsettled periods, with possible active conditions on 24 may.

This has been space weather, issued by XMDV radio at Thu the 23 May 2024 at 12:30:08

Space weather was created by William Greenwood with material from the N O double A

\ No newline at end of file