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Frontogenesis is the process by which fronts, separating fluids of different temperatures, are generated in the terrestrial atmosphere and oceans. It is of interest to consider whether this process appears in other planetary atmospheres. Here we analyse infra-red images taken by the Juno spacecraft at the Jovian poles and reveal ubiquitous vortices with a diameter of hundreds to thousands of kilometres and filaments with a width of tens of kilometres embedded in between the vortices. Our analysis shows that the filaments are dynamically active, reminiscent of terrestrial frontogenesis. Furthermore, our results indicate that Jovian frontogenesis acts in concert with moist convection, with the former mechanism favouring the development of cyclones and the latter the development of anti-cyclones. Even though moist convection is the main driver, frontogenesis accounts for a quarter of the total transfer of potential to kinetic energy, enhancing the upscale transfer of energy to larger vortices. Frontogenesis contributes 40% to the vertical heat transport, efficiently redistributing heat from Jupiter’s interior to its tropopause. This study highlights the broad range of interacting scales from tens to thousands of kilometres and the diverse physical mechanisms active at Jovian high latitudes.
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Data availability.
JIRAM data are available at the Planetary Data System (PDS) online ( https://atmos.nmsu.edu/PDS/data/PDS4/juno_jiram_bundle/data_calibrated/ ). Data products used in this study are the same as used in ref. 4 . They include calibrated, geometrically controlled, radiance data mapped onto an orthographic projection centred on the north pole and velocity vectors derived from the radiance data. Brightness maps and velocity vectors can be found in the supplementary data sets of ref. 4 .
The code is available at https://github.com/liasiegelman/JIRAM/blob/main/frontogenesis.py .
Bolton, S. J. et al. Jupiter’s interior and deep atmosphere: the initial pole-to-pole passes with the Juno spacecraft. Science 356 , 821–825 (2017).
Article ADS Google Scholar
Adriani, A. et al. Clusters of cyclones encircling Jupiter’s poles. Nature 555 , 216–219 (2018).
Moriconi, M. et al. Turbulence power spectra in regions surrounding Jupiter’s south polar cyclones from Juno/JIRAM. J. Geophys. Res. Planets 125 , e2019JE006096 (2020).
Siegelman, L. et al. Moist convection drives an upscale energy transfer at jovian high latitudes. Nat. Phys. 18 , 357–361 (2022).
Article Google Scholar
Siegelman, L., Young, W. R. & Ingersoll, A. P. Polar vortex crystals: emergence and structure. Proc. Natl Acad. Sci. USA 119 , e2120486119 (2022).
Article MathSciNet Google Scholar
Hoskins, B. J. & Bretherton, F. P. Atmospheric frontogenesis models: mathematical formulation and solution. J. Atmos. Sci. 29 , 11–27 (1972).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1972)029 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281972%29029%3C0011%3AAFMMFA%3E2.0.CO%3B2" aria-label="Article reference 6" data-doi="10.1175/1520-0469(1972)029 2.0.CO;2">Article ADS Google Scholar
Hakim, G. & Keyser, D. Canonical frontal circulation patterns in terms of Green’s functions for the Sawyer–Eliassen equation. Q. J. R. Meteorol. Soc. 127 , 1795–1814 (2001).
ADS Google Scholar
Capet, X., Klein, P., Hua, B. L., Lapeyre, G. & Mcwilliams, J. C. Surface kinetic energy transfer in surface quasi-geostrophic flows. J. Fluid Mech. 604 , 165–174 (2008).
Adriani, A. et al. Two-year observations of the Jupiter polar regions by JIRAM on board Juno. J. Geophys. Res. Planets 125 , e2019JE006098 (2020).
Lapeyre, G. Surface quasi-geostrophy. Fluids 2 , 7 (2017).
Juckes, M. Quasigeostrophic dynamics of the tropopause. J. Atmos. Sci. 51 , 2756–2768 (1994).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1994)051 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281994%29051%3C2756%3AQDOTT%3E2.0.CO%3B2" aria-label="Article reference 11" data-doi="10.1175/1520-0469(1994)051 2.0.CO;2">Article ADS Google Scholar
Juckes, M. Instability of surface and upper-tropospheric shear lines. J. Atmos. Sci. 52 , 3247–3262 (1995).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1995)052 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281995%29052%3C3247%3AIOSAUT%3E2.0.CO%3B2" aria-label="Article reference 12" data-doi="10.1175/1520-0469(1995)052 2.0.CO;2">Article ADS MathSciNet Google Scholar
Hakim, G. J., Snyder, C. & Muraki, D. J. A new surface model for cyclone–anticyclone asymmetry. J. Atmos. Sci. 59 , 2405–2420 (2002).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(2002)059 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%282002%29059%3C2405%3AANSMFC%3E2.0.CO%3B2" aria-label="Article reference 13" data-doi="10.1175/1520-0469(2002)059 2.0.CO;2">Article ADS MathSciNet Google Scholar
Lapeyre, G. & Klein, P. Impact of the small-scale elongated filaments on the oceanic vertical pump. J. Mar. Res. 64 , 835–851 (2006).
Lapeyre, G. & Klein, P. Dynamics of the upper oceanic layers in terms of surface quasigeostrophy theory. J. Phys. Oceanogr. 36 , 165–176 (2006).
Article ADS MathSciNet Google Scholar
Young, R. M. & Read, P. L. Forward and inverse kinetic energy cascades in Jupiter’s turbulent weather layer. Nat. Phys. 13 , 1135–1140 (2017).
Read, P. L. The dynamics of Jupiter’s and Saturn’s weather layers: a synthesis after Cassini and Juno. Annu. Rev. Fluid Mech. 56 , 271–293 (2023).
Achterberg, R. K. & Ingersoll, A. P. A normal-mode approach to jovian atmospheric dynamics. J. Atmos. Sci. 46 , 2448–2462 (1989).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1989)046 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281989%29046%3C2448%3AANMATJ%3E2.0.CO%3B2" aria-label="Article reference 18" data-doi="10.1175/1520-0469(1989)046 2.0.CO;2">Article ADS Google Scholar
Young, R. M., Read, P. L. & Wang, Y. Simulating jupiter’s weather layer. Part I: jet spin-up in a dry atmosphere. Icarus 326 , 225–252 (2019).
Shcherbina, A. Y. et al. Statistics of vertical vorticity, divergence, and strain in a developed submesoscale turbulence field. Geophys. Res. Lett. 40 , 4706–4711 (2013).
Balwada, D., Xiao, Q., Smith, S., Abernathey, R. & Gray, A. R. Vertical fluxes conditioned on vorticity and strain reveal submesoscale ventilation. J. Phys. Oceanogr. 51 , 2883–2901 (2021).
Hoskins, B. J. The mathematical theory of frontogenesis. Annu. Rev. Fluid Mech. 14 , 131–151 (1982).
Ingersoll, A., Gierasch, P., Banfield, D., Vasavada, A. & Team, G. I. Moist convection as an energy source for the large-scale motions in Jupiter’s atmosphere. Nature 403 , 630–632 (2000).
Gierasch, P. et al. Observation of moist convection in Jupiter’s atmosphere. Nature 403 , 628–630 (2000).
Vallis, G. K. Atmospheric and Oceanic Fluid Dynamics (Cambridge Univ. Press, 2017).
O’Neill, M. E., Emanuel, K. A. & Flierl, G. R. Polar vortex formation in giant-planet atmospheres due to moist convection. Nat. Geosci. 8 , 523–526 (2015).
Okubo, A. Horizontal dispersion of floatable particles in the vicinity of velocity singularities such as convergences. Deep Sea Res. Oceanogr. Abs. 17 , 445–454 (1970).
Weiss, J. The dynamics of enstrophy transfer in two-dimensional hydrodynamics. Physica D 48 , 273–294 (1991).
O’Neill, M. E., Emanuel, K. A. & Flierl, G. R. Weak jets and strong cyclones: shallow-water modeling of giant planet polar caps. J. Atmos. Sci. 73 , 1841–1855 (2016).
Hueso, R. & Sánchez-Lavega, A. A three-dimensional model of moist convection for the giant planets: the Jupiter case. Icarus 151 , 257–274 (2001).
Hueso, R., Sánchez-Lavega, A. & Guillot, T. A model for large-scale convective storms in Jupiter. J. Geophys. Res. Planets 107 , 5-1–5-11 (2002).
Sawyer, J. S. The vertical circulation at meteorological fronts and its relation to frontogenesis. Proc. R. Soc. London A 234 , 346–362 (1956).
Held, I. M., Pierrehumbert, R. T., Garner, S. T. & Swanson, K. L. Surface quasi-geostrophic dynamics. J. Fluid Mech. 282 , 1–20 (1995).
Thomas, L. N., Tandon, A. & Mahadevan, A. in Ocean Modeling in an Eddying Regime Vol. 177 (eds Thomas, L. N. et al.) 17–38 (American Geophysical Union, 2008).
Klein, P. & Lapeyre, G. The oceanic vertical pump induced by mesoscale and submesoscale turbulence. Annu. Rev. Mar. Sci. 1 , 351–375 (2009).
Pirraglia, J. Meridional energy balance of Jupiter. Icarus 59 , 169–176 (1984).
Li, L. et al. Less absorbed solar energy and more internal heat for Jupiter. Nat. Commun. 9 , 3709 (2018).
Adriani, A. et al. JIRAM, the Jovian infrared auroral mapper. Space Sci. Rev. 213 , 393–446 (2017).
Ferrari, R. A frontal challenge for climate models. Science 332 , 316–317 (2011).
Wolfe, C., Cessi, P., McClean, J. & Maltrud, M. Vertical heat transport in eddying ocean models. Geophys. Res. Lett. 35 , L23605 (2008).
Su, Z., Wang, J., Klein, P., Thompson, A. F. & Menemenlis, D. Ocean submesoscales as a key component of the global heat budget. Nat. Commun. 9 , 775 (2018).
Nastrom, G. & Gage, K. S. A climatology of atmospheric wavenumber spectra of wind and temperature observed by commercial aircraft. J. Atmos. Sci. 42 , 950–960 (1985).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1985)042 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281985%29042%3C0950%3AACOAWS%3E2.0.CO%3B2" aria-label="Article reference 42" data-doi="10.1175/1520-0469(1985)042 2.0.CO;2">Article ADS Google Scholar
Tulloch, R. & Smith, K. A theory for the atmospheric energy spectrum: depth-limited temperature anomalies at the tropopause. Proc. Natl Acad. Sci. USA 103 , 14690–14694 (2006).
Waite, M. L. & Snyder, C. Mesoscale energy spectra of moist baroclinic waves. J. Atmos. Sci. 70 , 1242–1256 (2013).
Burgess, B. H., Erler, A. R. & Shepherd, T. G. The troposphere-to-stratosphere transition in kinetic energy spectra and nonlinear spectral fluxes as seen in ECMWF analyses. J. Atmos. Sci. 70 , 669–687 (2013).
Hamilton, K., Takahashi, Y. O. & Ohfuchi, W. Mesoscale spectrum of atmospheric motions investigated in a very fine resolution global general circulation model. J. Geophys. Res. Atmos. 113 , 110–129 (2008).
Rubio, A. M., Julien, K., Knobloch, E. & Weiss, J. B. Upscale energy transfer in three-dimensional rapidly rotating turbulent convection. Phys. Rev. Lett. 112 , 144501 (2014).
Julien, K., Rubio, A. M., Grooms, I. & Knobloch, E. Statistical and physical balances in low rossby number Rayleigh–Bénard convection. Geophys. Astrophys. Fluid Dyn. 106 , 392–428 (2012).
Favier, B., Silvers, L. & Proctor, M. Inverse cascade and symmetry breaking in rapidly rotating Boussinesq convection. Phys. Fluids 26 , 096605 (2014).
Guervilly, C., Hughes, D. W. & Jones, C. A. Large-scale-vortex dynamos in planar rotating convection. J. Fluid Mech. 815 , 333–360 (2017).
Ingersoll, A. P. et al. Vorticity and divergence at scales down to 200 km within and around the polar cyclones of Jupiter. Nat. Astron. 6 , 1280–1286 (2022).
Orszag, S. A. Numerical simulation of incompressible flows within simple boundaries: accuracy. J. Fluid Mech. 49 , 75–112 (1971).
Charney, J. G. Geostrophic turbulence. J. Atmos. Sci. 28 , 1087–1095 (1971).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1971)028 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281971%29028%3C1087%3AGT%3E2.0.CO%3B2" aria-label="Article reference 53" data-doi="10.1175/1520-0469(1971)028 2.0.CO;2">Article ADS Google Scholar
Blumen, W. Uniform potential vorticity flow: part I. Theory of wave interactions and two-dimensional turbulence. J. Atmos. Sci. 35 , 774–783 (1978).
2.0.CO;2" data-track-item_id="10.1175/1520-0469(1978)035 2.0.CO;2" data-track-value="article reference" data-track-action="article reference" href="https://doi.org/10.1175%2F1520-0469%281978%29035%3C0774%3AUPVFPI%3E2.0.CO%3B2" aria-label="Article reference 54" data-doi="10.1175/1520-0469(1978)035 2.0.CO;2">Article ADS Google Scholar
Lapeyre, G. What vertical mode does the altimeter reflect? On the decomposition in baroclinic modes and on a surface-trapped mode. J. Phys. Oceanogr. 39 , 2857–2874 (2009).
Holton, J. R. (ed.) An Introduction to Dynamic Meteorology Vol. 88 (Elsevier Academic, 2004).
Hua, B. L., McWilliams, J. C. & Klein, P. Lagrangian accelerations in geostrophic turbulence. J. Fluid Mech. 366 , 87–108 (1998).
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We thank T. Ewald for processing the infra-red images taken by JIRAM used in this study and W. Young for insightful discussions. L.S. is supported by the National Science Foundation (OCE-1657041). P.K. acknowledges funding from JPL/NASA.
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Lia Siegelman
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Patrice Klein
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Extended data fig. 1 cumulative integrals of χ..
Same as Fig. 4 for \(\tilde{{\chi }^{+}}/\overline{{\chi }^{+}}\) (red curve) and \(\tilde{{\chi }^{-}}/\overline{{\chi }^{-}}\) (blue curve). The dotted line shows the fractional area as a function of \({{{{\rm{d}}}}}_{\max }/{{{\rm{d}}}}\) , with d the vorticity-strain JDF and \({{{{\rm{d}}}}}_{\max }\) its maximum, χ + are updrafts and χ − downdrafts. \(\overline{{\chi }^{+}}\) and \(\overline{{\chi }^{-}}\) have equal magnitude of 0.3 f . The shaded envelopes indicate the range of results obtained with the different low-pass Butterworth filters (see error section in the Methods ). This figure confirms the asymmetry observed in the strain-vorticity space (Fig. 3c ). For instance, scales larger than 230 km, which occupy half of the domain, capture a little over 50% of the χ + but only 10% of the χ − . Similarly, scales smaller than 150 km, which occupy twenty percent of the domain, capture almost 60% of the χ − but only about 20% of χ + . In summary, positive divergence is localized in a large fraction of the physical space and corresponds to large length scales, whereas negative divergence is scattered throughout the domain, occupies a small fraction of the physical space, and corresponds to small length scales.
Wavenumber spectrum of vorticity ζ used in this paper (thick black curve) and wavenumber spectra of divergence χ (thin colored curves) derived after filtering the wind velocities derived from feature tracking with a low-pass Butterworth filter of order n and wavelength cutoff w cutoff . The spectra of ζ is used a an upper bound for the derivation of χ . χ used in the study corresponds to the low-pass Butterworth filter of order 1 and cutoff wavelength of 250 km (green curve, see error section in the Methods ).
Error propagation analysis in wind velocities derived from feature tracking. Each panel shows the weighted JDF of χ /f in vorticity-strain space, with χ the divergence derived after application of a low-pass Butterworth of order n and cutoff wavelength w cutoff and f the Coriolis parameter. The dashed lines are the ∣ ζ ∣ = σ lines, with ζ the vorticity and σ strain. a ) n = 5, w cutoff = 50 km; b ) n = 5, w cutoff = 100 km; c ) n = 1, w cutoff = 250 km, d ) n = 1, w cutoff = 300 km, e ) n = 2, w cutoff = 300 km, f ) n = 2, w cutoff = 500 km. Panel c corresponds to Fig. 3c in the main text. The dispersion in panel a indicates that scales ≤ 50 km contain too much noise. All other panels yield comparable results indicating that the effective resolution of the divergence is between 50 and 100 km (see error section in the Methods for more details).
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Siegelman, L., Klein, P. Frontogenesis at Jovian high latitudes. Nat. Phys. (2024). https://doi.org/10.1038/s41567-024-02516-x
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This package implements several hypothesis tests in Julia.
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Hypothesis testing is a technique used by statisticians, scientists and data analysts for measuring whether the results of an experiment are meaningful and reliable. The statistical significance of the results of an experiment is often quantified using a P-value. This tutorial aims to build intuition for hypothesis testing using some real-world ...
Solution: Assuming the null hypothesis H_0 H 0 is true. Throwing a coin is the perfect example of a bernoulli distribution. Which is why we can directly use the formula for standard deviation. \sigma = \sqrt {p (1-p)} σ = p(1 −p) Now, let's calculate the z-statistic: Collaborate with prasanthi-vvit on hypothesis-testing-solutions notebook.
Hypothesis testing is used to confirm your conclusion (or hypothesis) about the population parameter (which you know from EDA or your intuition). Through hypothesis testing, you can determine whether there is enough evidence to conclude if the hypothesis about the population parameter is true or not. Q - Null and Alternate Hypotheses.
Collaborate with theashishgoyal on hypothesis-testing notebook. Sign In. Learn practical skills, build real-world projects, and advance your career. ... Chi-Square Test-The test is applied when you have two categorical variables from a single population. It is used to determine whether there is a significant association between the two variables.
In today's blog post, we will discuss the various types of hypothesis testing that help data scientists develop the right judgments and make better decisions. #datascientists #testing https://lnkd ...
Present the findings in your results and discussion section. Though the specific details might vary, the procedure you will use when testing a hypothesis will always follow some version of these steps. Table of contents. Step 1: State your null and alternate hypothesis. Step 2: Collect data. Step 3: Perform a statistical test.
Unit 12: Significance tests (hypothesis testing) Significance tests give us a formal process for using sample data to evaluate the likelihood of some claim about a population value. Learn how to conduct significance tests and calculate p-values to see how likely a sample result is to occur by random chance. You'll also see how we use p-values ...
6. Test Statistic: The test statistic measures how close the sample has come to the null hypothesis. Its observed value changes randomly from one random sample to a different sample. A test statistic contains information about the data that is relevant for deciding whether to reject the null hypothesis or not.
It tests the null hypothesis that the population variances are equal (called homogeneity of variance or homoscedasticity). Suppose the resulting p-value of Levene's test is less than the significance level (typically 0.05).In that case, the obtained differences in sample variances are unlikely to have occurred based on random sampling from a population with equal variances.
Hypothesis testing is a statistical method to determine whether a hypothesis that you have holds true or not. The hypothesis can be with respect to two variables within a dataset, an association between two groups or a situation. The method evaluates two mutually exclusive statements (two events that cannot occur simultaneously) to determine ...
Learn more about installing Jovian python library and some of the core features of Jovian. Run this command in your terminal: pip install jovian -q --upgrade. Automate building, versioning, and hosting of your technical documentation continuously on Read the Docs.
The null hypothesis represented as H₀ is the initial claim that is based on the prevailing belief about the population. The alternate hypothesis represented as H₁ is the challenge to the null hypothesis. It is the claim which we would like to prove as True. One of the main points which we should consider while formulating the null and alternative hypothesis is that the null hypothesis ...
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The process of hypothesis testing based on the traditional method includes calculating the critical value, testing the value of the test statistic… Hypothesis: Accept or Fail to Reject? The outcome of any hypothesis testing leads to rejecting or not rejecting the null hypothesis. This decision is taken based on the analysis of the…
Image by Author. We reject the null hypothesis(H₀) if the sample mean(x̅ ) lies inside the Critical Region.; We fail to reject the null hypothesis(H₀) if the sample mean(x̅ ) lies outside the Critical Region.; The formulation of the null and alternate hypothesis determines the type of the test and the critical regions' position in the normal distribution.
Perspective. Our results suggest that frontogenesis is an active mechanism at Jovian high latitudes. The importance of frontogenesis is, however, probably underestimated, since the downdrafts ...
Hypothesis Testing Solutions. This is a solution notebook for the Hypothesis Testing tutorial notebook by Aakash NS. import math from scipy.stats import norm. EXERCISE: A coin is tossed 1000 times and results in 476 heads. Is the coin biased? Use a significance level of 0.01. Solution:
HypothesisTests package. This package implements several hypothesis tests in Julia. Methods. Confidence interval. p-value. Parametric tests. Power divergence test. Pearson chi-squared test. Multinomial likelihood ratio test.
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