Recommended Posts

if you mean me, i dont have the tools to create them

no special tools required ;)

download the qmup release i had done. check out how my modules are organized. then use apv6 modules of the ones you do. the conversion from apv5 to apv6 modules can be done with the latest module editor (2.0.7 i think). then just edit the modules to make the names short (as i did, only keeping the kb123456 part).

Is there any chance of getting AutoPatcher QMUP's for the months of September and October?

BTW, here's August (full) for those still looking...

http://www.9down.com/story.php?sid=7095

On a side note...have you guys heard that XP SP3 has been moved way back to some time in 2008!?!

http://www.microsoft.com/windows/lifecycle/servicepacks.mspx

Edited by alceryes

http://ap.manroweb.co.uk/index_QMUP.html

I have created and uploaded AutoPatcher XP/2003/2000 QMUP October Builds.

AutoPatcher_XP_Oct2006_English_QMUP.exe

File Size: 12.1 MB (12,736,798 bytes)

MD5 Hash: 77BB399676CE0FAEF0411F39FDECD1B7

AutoPatcher_2003_Oct2006_English_QMUP.exe

File Size: 9.37 MB (9,828,118 bytes)

MD5 Hash: B0D3E54F441282280294EE403EF3FF70

AutoPatcher_2000_Oct2006_English_QMUP.exe

File Size: 8.55 MB (8,966,857 bytes)

MD5 Hash: 35A4FFD99498AF38297311880A76776A

Please test this build and let me know of any problems.

http://ap.manroweb.co.uk/index_QMUP.html

Edited by itsnotmeeee

http://ap.manroweb.co.uk/index_QMUP.html

I have created and uploaded AutoPatcher XP/2003/2000 QMUP October Builds.

AutoPatcher_XP_Oct2006_English_QMUP.exe

File Size: 12.1 MB (12,736,798 bytes)

MD5 Hash: 77BB399676CE0FAEF0411F39FDECD1B7

AutoPatcher_2003_Oct2006_English_QMUP.exe

File Size: 9.37 MB (9,828,118 bytes)

MD5 Hash: B0D3E54F441282280294EE403EF3FF70

AutoPatcher_2000_Oct2006_English_QMUP.exe

File Size: 8.55 MB (8,966,857 bytes)

MD5 Hash: 35A4FFD99498AF38297311880A76776A

Please test this build and let me know of any problems.

http://ap.manroweb.co.uk/index_QMUP.html

Please note the MD5 Hashes have changed due a small update in the builds

Check http://ap.manroweb.co.uk/index_QMUP.html for upto date file hash

Excellent, Thank You!!

...any chance of getting a Sept. QMUP?

- August 06 full

- September 06 QMUP

- October 06 QMUP

That way all of us noobs will only have to go through installing all the extra programs and settings once. I know we might miss out on a few program updates but it's mainly the security flaw fixes I want.

TIA...

Excellent, Thank You!!

...any chance of getting a Sept. QMUP?

- August 06 full

- September 06 QMUP

- October 06 QMUP

That way all of us noobs will only have to go through installing all the extra programs and settings once. I know we might miss out on a few program updates but it's mainly the security flaw fixes I want.

TIA...

Sept and Oct QMUP > http://ap.manroweb.co.uk/index.html

I will endeavour to do Nov as soon as the patches are released, and assuming the autopatcher team have no issues with me doing so.

Please feedback any problems you encounter with any of the QMUP downloads

  • 4 weeks later...

I think for QMUP's to be useful they need to include Critical, Recommended, and Add-ons that have been updated since last month.

For example, I wouldn't want to install just Critical updates if there are 6-7 Recommended updates as well. And, I certainly wouldn't want to deploy QMUP's on a month when IE7 is released since I want to be able to deploy that as well.

My point is, QMUP's could attract a much broader audience if they were tweaked to be comprehensive... in the month that they are covering.

  • 1 month later...
  • 1 month later...
  • 4 weeks later...

itsnotmeeee

Ill get Jan07 done for tomorrow!

Not sure how many people are using it at present, so not sure if we should continue with it.

If you are using QMUP's and want to see this continue then please do contact me or reply here

Personally I think the QMUP's are a great idea for updating systems already patched from the previous month .

Although it's essential to have a Full/Lite Release , and the consecutive monthly updates , if you have a bunch of Comps

and want to quickly update them all offline securely latest QMUP is a very handy tool.

It's your call obviously :)

This topic is now closed to further replies.
  • Recently Browsing   0 members

    • No registered users viewing this page.
  • Posts

    • It's amazing that anyone still uses this bloated trash.
    • @Sayan...I have defended you at various points as I hope you know. This headline however is utter trash...shame on you sir!
    • An actual cosmic "Eye of Sauron" had been looking straight at us all along by Sayan Sen Image by Kovin P. Vasquez via Pexels | Not representative An international team of researchers has solved a long-standing mystery surrounding a distant blazar known as PKS 1424+240, helping explain why it produces some of the brightest high-energy gamma rays and cosmic neutrinos ever observed despite appearing to have a relatively slow-moving jet. The findings were published on June 6 in Astronomy & Astrophysics Letters. The study addresses a broader challenge in astrophysics: understanding how extreme cosmic objects accelerate particles to very high energies and produce very high-energy (VHE) photons and neutrinos. PKS 1424+240 is located billions of light-years from Earth. It has attracted attention for years because it is both a powerful source of VHE gamma rays and the brightest known neutrino-emitting blazar in the sky, according to observations by the IceCube Neutrino Observatory. It is also associated with one of the strongest peaks in IceCube's nine-year neutrino sky map A blazar is a type of active galactic nucleus powered by a supermassive black hole that pulls in surrounding matter and launches jets of plasma moving close to the speed of light. What makes blazars unique is their orientation. One of their jets points almost directly toward Earth, making them appear exceptionally bright across the electromagnetic spectrum and allowing scientists to study some of the most extreme physical processes in the Universe. The scientists exclaimed it's like the 'Eye of Sauron' in deep space. Usually, the brightest gamma-ray-emitting blazars are expected to have jets that appear to move very quickly. However, radio observations of PKS 1424+240 suggested that its jet was moving much more slowly, creating a contradiction that became part of a long-running problem known as the "Doppler factor crisis." To investigate, researchers analyzed 15 years of observations from the Very Long Baseline Array (VLBA), a network of 10 radio antennas spread across the continental United States, Hawaii and St. Croix. Using a technique called Very Long Baseline Interferometry (VLBI), astronomers combine signals from widely separated radio telescopes to create a virtual Earth-sized telescope capable of revealing extremely fine details. The team combined 42 polarization-sensitive radio images collected between 2009 and 2025, creating a much deeper and more detailed view of the jet than had previously been possible. The observations were carried out as part of MOJAVE (Monitoring Of Jets in Active galactic nuclei with VLBA Experiments), a long-running program that studies the brightness, polarization and magnetic field structures of jets produced by active galaxies. The project aims to better understand how activity near supermassive black holes is linked to high-energy radiation and neutrino emission. “When we reconstructed the image, it looked absolutely stunning,” said Yuri Kovalev, lead author of the study and Principal Investigator of the European Research Council-funded MuSES project at the Max Planck Institute for Radio Astronomy. “We have never seen anything quite like it — a near-perfect toroidal magnetic field with a jet, pointing straight at us.” The image revealed an unusual geometry. The researchers found that Earth lies almost directly in line with the jet, with a viewing angle of less than 0.6 degrees. In simple terms, astronomers are looking almost straight down the jet. This turned out to be the key to the mystery. Because the jet is aimed almost directly at Earth, a relativistic effect called Doppler boosting dramatically increases its apparent brightness. The study found that this effect boosts the emission by a factor of about 30 while also making the jet appear slower than it actually is. “This alignment causes a boost in brightness by a factor of 30 or more,” said Jack Livingston, a co-author at the Max Planck Institute for Radio Astronomy. “At the same time, the jet appears to move slowly due to projection effects — a classic optical illusion.” The nearly head-on view also gave scientists a rare look at the jet's magnetic field. Using polarized radio signals, they detected a clear toroidal, or doughnut-shaped, magnetic field component. The observations suggest the jet carries an electric current and that its magnetic field helps launch, shape and stabilize the flow of plasma. Researchers believe this magnetic structure may also play a key role in accelerating particles to energies high enough to produce both gamma rays and neutrinos. “Solving this puzzle confirms that active galactic nuclei with supermassive black holes are not only powerful accelerators of electrons, but also of protons — the origin of the observed high-energy neutrinos,” Kovalev said. The research was conducted under the MuSES (Multi-messenger Studies of Energetic Sources) project, which investigates how active galactic nuclei accelerate particles and generate different cosmic signals, including light and neutrinos. Scientists say understanding how protons are accelerated and linked to neutrino production remains one of the major unanswered questions in astrophysics. The findings help explain why some blazars can appear to have slow jets while still producing extremely bright high-energy emissions. More broadly, the study strengthens the link between relativistic jets, magnetic fields, gamma rays and high-energy neutrinos. Researchers say the results provide new clues about how some of the Universe's most powerful natural particle accelerators work and offer important insights for multimessenger astronomy, which combines different types of cosmic signals to study extreme events in space. Source: European Research Council, EDP Sciences This article was generated with some help from AI and reviewed by an editor. Under Section 107 of the Copyright Act 1976, this material is used for the purpose of news reporting. Fair use is a use permitted by copyright statute that might otherwise be infringing.
    • Gotenks98 is right... Outlook (new) is absolute trash. Doesn't Mozilla have an Enterprise Version of Firebird?
  • Recent Achievements

    • One Month Later
      lamborghiniv10 earned a badge
      One Month Later
    • Week One Done
      lamborghiniv10 earned a badge
      Week One Done
    • Reacting Well
      X-No-file earned a badge
      Reacting Well
    • One Month Later
      pestcontrol46 earned a badge
      One Month Later
    • Week One Done
      pestcontrol46 earned a badge
      Week One Done
  • Popular Contributors

    1. 1
      +primortal
      511
    2. 2
      PsYcHoKiLLa
      273
    3. 3
      Skyfrog
      75
    4. 4
      +Edouard
      72
    5. 5
      FloatingFatMan
      68
  • Tell a friend

    Love Neowin? Tell a friend!