11
submitted 1 week ago by f1ip@lemmy.world to c/formula1@lemmy.world

The rumour mill is spinning like crazy that Red Bull will announce RIC's gone then 10 minutes later that Lawson is in.

And there is the not-always-reliable Joe Savard soying PER will announce he is leaving after Mexico. [link] (https://joesaward.wordpress.com/2024/09/26/green-notebook-from-somerset/)

[-] f1ip@lemmy.world 6 points 1 week ago

No one can trust Red Bull, obviously, but yes, that is the rumour.

But this is one of those situations where I hope both sides lose (the team's other personnel is the sad collateral damage, which sucks). So if RBR can be in the low midfield next season and then both Horner and Marko get the sack, that would be splendid.

[-] f1ip@lemmy.world 10 points 1 week ago

The exodus continues. Behind the smiles and jokes in the press conferences, the atmosphere must be horrendously bad for top, middle, and bottom people be heading for the exits as if the ship is sinking.

Low-key hoping next year is humbling for Horner and Marko. A pity for everyone else that works there, but those two really needs a swift kick in the arse.

17
submitted 1 week ago by f1ip@lemmy.world to c/formula1@lemmy.world

Updated the qualy battles plot, but did not want to burden the servers with it, so if you want to see a gif from the start to Singapore, here it is: https://i.imgur.com/KrbkqQF.gif.

And now we wait for the avalanche of stupid/crazy/ridiculous rumours about RIC until the next race.

[-] f1ip@lemmy.world 6 points 1 week ago

The king of malicious compliance. And one of the best Brooklyn 99 guest stars.

[-] f1ip@lemmy.world 23 points 1 week ago

I love it. Malicious compliance is the best form of protest. To hell with MbS (both of them, actually).

20
submitted 1 week ago by f1ip@lemmy.world to c/formula1@lemmy.world

Featuring Albon, Tsunoda, and Verstappen. Yet, here we are.

Telemetry Comparisons and Track Dominance plots

And, if you want to help me out, here are many Track Dominance graphics with different mini-sectors (numbers are under the images in the link): varied track dominance graphics What do you think is the most useful to understand where each car goes better?

[-] f1ip@lemmy.world 4 points 2 weeks ago

I think one of the issues he was adamant about was no 1 year deal. So I would guess he is at least 2 years.

But Audi has a vacant seat...

27
submitted 2 weeks ago by f1ip@lemmy.world to c/formula1@lemmy.world

Verstappen and Albon finally lost one this season!!!

Yes, Albon was pretty severely compromised in the last Q3 attempt by extra weight on his car, but still here we are. Williams and Red Bull no longer have zeros on the board (sorry, Logan, you remain at zero).

21
submitted 3 weeks ago by f1ip@lemmy.world to c/formula1@lemmy.world

With a 30 points lead over Hamilton for points scored at Baku, Pérez will retain his lead, no matter what happens.

But with the current competitive state of the Red Bulls in tracks with slow corners, the lead could suffer a dent if Hamilton has a good weekend.

If Norris has a good weekend, he could jump a few spots, and Piastri could finally enter into the conversation, as he failed to score a point in 2023.

[-] f1ip@lemmy.world 4 points 3 weeks ago

Last part of the paper:

For stellar models, the remarkably high 𝜉ion is untenable 27,36 under common initial mass functions (IMFs). Since this quantity is directly sensitive to the hottest stars, its extreme value may be ascribed to an extension of the IMF to very massive stars 37,38. The high average ionising-photon energy of a 𝑇 = 105 K blackbody moreover yields a 2× higher ratio of Lyα to LyC photons than standard case-B recombination24, thereby bringing the required 𝜉ion more closely in agreement with the theoretical maximum for such stars 39. Whilst at such high 𝜉ion (and relatively low 𝑓esc, LyC) a UV turnover could be produced by a prominent nebular continuum40, the extremely blue UV continuum (𝛽UV ≲ −2.7) appears incompatible with a 2𝛾- dominated spectrum. One explanation is to invoke an ISM density upwards of 𝑛 ≈ 104 cm−3, as may be expected from the compactness of JADES-GS-z13-1-LA. Considering nebular continuum would be reddened further by the free-bound contribution, however, it may again indicate significant LyC leakage, corroborating the suggestion that JADES-GS-z13-1-LA is located inside an ionised bubble.

One particularly intriguing class of objects predicted to radiate up to 40% of their bolometric luminosity as Lyα are entirely metalfree Population III (Pop III) stars 41–43 thought to reach significantly higher masses and effective temperatures than subsequent metal-4 enriched stellar populations. However, the absolute UV magnitude of JADES-GS-z13-1-LA, 𝑀UV ≈ −18.7 mag, would require a stellar mass of 𝑀∗ ≈ 106 M⊙ as a pure Pop III system, somewhat higher than typical predictions 44. We further note the absence of strong He ii 𝜆 1640 Å emission (Methods) may argue against the Pop III scenario45, although its strength rapidly evolves a few Myr after a star formation burst 42,43. A high LyC escape fraction would also suppress He ii, yet still leaves the UV turnover to be explained.

Whatever the origin of the Lyα emission of JADES-GS-z13-1-LA may be, it reveals the rather extreme character of one of the earliest galaxies known, despite having been found in a modest survey area 16 probing a comoving volume of 50 000 Mpc3 between 𝑧 = 11 and 𝑧 = 15. At just 330 Myr after the Big Bang, JADES-GS-z13-1-LA indicates the profound marks left on the IGM by the first generation of galaxies through the creation of reionised regions. Furthermore, it provides tangible evidence for the Wouthuysen-Field coupling of the spin temperature of neutral hydrogen to that of the gas via the emission of Lyα photons, the global evolution of which is anticipated to be uncovered soon by H i 21 cm experiments 46,47 to provide a complementary view of Cosmic Dawn.

Sadly, no mention of the obvious reason for this: aliens!

47
submitted 3 weeks ago by f1ip@lemmy.world to c/formula1@lemmy.world

Anyone else surprised at the short gardening leave? Him starting in March changes things. I thought he would be out at least until September of 2025,which would hurt his participation in the 2026 design. If, however, he does start in March, he can absolutely be a major part of the redesign and that changes the calculations for who might be a force in 2026.

14
submitted 3 weeks ago by f1ip@lemmy.world to c/discworld@lemmy.ml

There are many ways to read the series, obviously, so I am curious as to what are people's preferred method.

I read them chronologically by publishing date the first time, then once by theme (Watch, Witches, and Moist novels first) and then been reading books here and there kinda randomly (although when I read one Watch novel, I tend to read all of them to the end, plus Raising Steam).

What do others do?

[-] f1ip@lemmy.world 7 points 3 weeks ago

The way the graphic is presented, it does look like it is a count of this season only.

VER has almost 100 points scored in Monaco alone in his career and LEC has 100 in Jeddah and Baku added up, for example.

[-] f1ip@lemmy.world 6 points 3 weeks ago

Which is my point. Five out of 19 never made it and this year is looking doubtful (even with all the Audi rumours). Plus, once the driver academies came into being, winning F2 at the wrong time is a problem. Piastri being the clearest example, Alpine screwed up and he only made it to F1 because they are a terribly run team and McL poached him.

And fairness is an irrelevant concept in sports, there is no fairness and there never was. If there was, Jacques Villeneuve would have been kicked out of motorsports once he released his album.

[-] f1ip@lemmy.world 19 points 3 weeks ago

When has fairness ever happened in F1? It is all a factor of who you aligned yourself with.

Pourchaire was in the Sauber academy, Sauber academy is a mess, he pays the price. It has nothing to do with fairness or worth or who won what. How many F2 champions have never even sniffed an F1 seat?

[-] f1ip@lemmy.world 7 points 3 weeks ago

There was really no other option, considering more track time for the team's 2025 driver can only help. Just hope he has another good—meaning uneventful—weekend.

[-] f1ip@lemmy.world 7 points 4 weeks ago

MbS really tried to play with the big boys in F1 and got 100% wrecked. Nothing went the way he wanted and now he has even less power over the series.

Good job, president!

28
submitted 4 weeks ago by f1ip@lemmy.world to c/formula1@lemmy.world

I have been toying around with F1 data and python plots, and got some average gap graphics in gif form, starting at Bahrain and up to Italy.

They are gifs, so check your wi-fi upon entering because there are many on each page, obviously.

Would have posted a few examples here, but apparently Lemmy is not keen on it. Hope imgur's servers do not crap out on me.

Examples:

[-] f1ip@lemmy.world 4 points 4 weeks ago

167 laps for Bearman (Wet and Inter), 76 laps for Lawson (Inters and slicks before the issue ended his day).

15
submitted 4 weeks ago by f1ip@lemmy.world to c/formula1@lemmy.world

Main points of the article:

Pirelli ran two tests of the 2025 tyres, one in Monza with Red Bull's junior team, one in Fiorano with Ferrari. It was wet in Monza and Lawson had some PU trouble in the VCARB01, while Fiorano was artificially wet for Bearman in the Ferrari.

Next up, Aston Martin will be the first to test the 2026 tyres at Barcelona after the Baku GP and then Mercedes at Magny-Cours with the 2025 tyres (1-2 October).


The irony of Fiorano being artificially wet and it was just raining in Monza is pretty great, yes.

Also, great practice for Bearman if he will indeed be in Baku in place of Magnussen.

view more: next ›

f1ip

joined 1 month ago